Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-14T13:01:25.817746Z
Paper Citation Record · LEDGER
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars
As of 16 August 2026, this Paper Citation Record lists 100 of 126 outbound references and 0 inbound Pith citation observations for arXiv:1908.06104.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
100 of 126 outbound references displayed
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- verified fuzzy35
- unresolved58
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External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 3d0d49bb-ce26-49f4-b908-9d76b3df94c4 · outbound
This paper cites 2018, AJ, 156, 294 (A19).
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2018, AJ, 156, 294 (A19)
Reference 1
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.475476Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3186d24e-0067-41d1-b757-88e69451af56 · outbound
This paper cites 2017, MNRAS, 472, 591.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2017, MNRAS, 472, 591
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.479722Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 6bf340e3-f3a9-414e-9096-fcb5d86edbac · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 3
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.483598Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation acef0d0e-2219-4d3d-9b98-66867e2cb6a8 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.487583Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7ca15967-9a5c-4aa5-a3f3-c7776f85f021 · outbound
This paper cites 1989, ARA&A, 27, 629.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1989, ARA&A, 27, 629
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.491755Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a9075ca0-757f-4832-883e-544b0f0dff3d · outbound
This paper cites 2019, MNRAS, 486, 266.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2019, MNRAS, 486, 266
Reference 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.495256Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b481154e-f987-4f61-8174-1f25e5f3316f · outbound
This paper cites 1961, BAN, 15, 265.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1961, BAN, 15, 265
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.498887Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9754e013-4788-4518-a312-94f737294361 · outbound
This paper cites 1964, ARAA, 2, 213.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1964, ARAA, 2, 213
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.501966Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e8ce9e9f-c17d-4b79-90b1-f52a451f99fc · outbound
This paper cites 2016, MNRAS, 458, 1999.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2016, MNRAS, 458, 1999
Reference 9
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.505178Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7f16e3fd-44a8-4e45-ad76-4a632a96a880 · outbound
This paper cites 1959, ApJ, 130, 482.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1959, ApJ, 130, 482
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.509470Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 431f88f4-e587-4e6b-93f8-a857cb0e0c63 · outbound
This paper cites 1997, in.
Reference 11
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c5f725eb-63a0-4cd0-9bd0-1a6b887e9ce3 · outbound
This paper cites 2005, A&A, 438, 301.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2005, A&A, 438, 301
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.516741Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 158b10d8-7c4b-4108-a79a-ecaa6a8ba5d2 · outbound
This paper cites J., Hunter, I., et al.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars J., Hunter, I., et al
Reference 13
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.519745Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 54d622f5-0a98-4c40-8b8a-b8023fb0ef46 · outbound
This paper cites 1976, Mem.\ Soc.\ R.\ Sci.\ Lie'ge, 9, 193.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1976, Mem.\ Soc.\ R.\ Sci.\ Lie'ge, 9, 193
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.522716Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 63f67a26-994c-4de8-921d-f9458dfefc39 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 15
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.525782Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e3e231cf-a133-433e-8c50-2cd1be011898 · outbound
This paper cites 2006, A&A, 446, 279.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2006, A&A, 446, 279
Reference 16
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.528526Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 20f1b3f7-ec12-4c6c-8bf0-1bb985acc521 · outbound
This paper cites 2007, ARAA, 45, 177.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2007, ARAA, 45, 177
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.531777Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2b336213-06da-48ce-83ab-1c6cab23bb9c · outbound
This paper cites 2008, Asp Conf Ser, 388, 109.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2008, Asp Conf Ser, 388, 109
Reference 18
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.534612Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 0fd85f81-9ab4-4786-9c7e-6adfc7007392 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 19
- Resolution
- parse uncertain
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5020f75a-367b-4acc-ac88-e8951943c6cf · outbound
This paper cites Phys., Conf.\ Ser., 318, 012022.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Phys., Conf.\ Ser., 318, 012022
Reference 20
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.541462Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 1398f1c2-9213-4cbf-9f9e-647f128956e0 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.544363Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 82b8ffe7-0203-4cc9-94b0-9b732f952cf9 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 22
- Resolution
- parse uncertain
- no resolver link, observed 2026-08-14T13:01:25.547731Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 36c6a7f9-ccfd-4be3-9d69-0a0de20dcea7 · outbound
This paper cites 2012, A&A, 537, A146.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2012, A&A, 537, A146
Reference 23
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.551298Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 181b49e0-c4a9-4327-ac1c-0b5c1a58f669 · outbound
This paper cites 2008, MNRAS, 384, 1109.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2008, MNRAS, 384, 1109
Reference 24
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.554379Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8f39c190-13ee-4cb7-a788-eb205db85f71 · outbound
This paper cites 2011, MNRAS, 414, 3501.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2011, MNRAS, 414, 3501
Reference 25
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.558338Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b6cdb290-65bf-4284-9375-ffa9d52745e6 · outbound
This paper cites 2017, PASA, 34, 58.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2017, PASA, 34, 58
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.562024Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3e7c0079-1b62-45e7-929e-ab96f40d14b8 · outbound
This paper cites 2007, A&A, 464, 289.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2007, A&A, 464, 289
Reference 27
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.565480Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7e15c664-e626-4993-8240-834584934fc5 · outbound
This paper cites 2019, A&A, 621, A22.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2019, A&A, 621, A22
Reference 28
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.569421Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a1d75fe8-ad8a-4461-adec-3b94b52e78b5 · outbound
This paper cites 1990, ApJ, 363, 119.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1990, ApJ, 363, 119
Reference 29
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.574187Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 38fd24b2-59cb-41f7-a1ae-ee170bc42e56 · outbound
This paper cites 1996, ApJ, 469, 355.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1996, ApJ, 469, 355
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.577721Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3993e60e-066c-4ab8-ac18-0a8ce96053c4 · outbound
This paper cites 2006, ApJ, 637, 1025.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2006, ApJ, 637, 1025
Reference 31
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.582017Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation be9a957e-164d-473d-be71-84ea28127311 · outbound
This paper cites K.\ Davidson, A.F.J.\ Moffat, & H.J.G.L.M.\ Lamers (Dordrect: Kluwer), 185.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars K.\ Davidson, A.F.J.\ Moffat, & H.J.G.L.M.\ Lamers (Dordrect: Kluwer), 185
Reference 32
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ce9c5631-b78d-4a63-9cec-21b698685242 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.590631Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b25be5d2-d8a1-4247-bcb6-9fe2b18191bd · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 34
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f514088e-d0fb-45ec-8679-0b01d3ac457d · outbound
This paper cites 1982, ApJ, 263, 777.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1982, ApJ, 263, 777
Reference 35
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.597716Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 82b172a1-5d75-43cf-9269-6208cd0015a2 · outbound
This paper cites 1987, ApJS, 64, 545.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1987, ApJS, 64, 545
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.600755Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c48574bc-5c47-4313-bb92-1b5bd6a4dd7f · outbound
This paper cites 2017, A&A, 608, 11.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2017, A&A, 608, 11
Reference 37
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.603722Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation dd61895a-83e3-4046-b680-f4298af8301b · outbound
This paper cites 2018, A&A, 615, A78.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2018, A&A, 615, A78
Reference 38
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.607230Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e4d1ebab-523c-447e-a90d-a6aaa1f7d69a · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 39
- Resolution
- parse uncertain
- no resolver link, observed 2026-08-14T13:01:25.611082Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 8848cd9a-7e9b-4938-9e12-730b3fce1b01 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 40
- Resolution
- parse uncertain
- no resolver link, observed 2026-08-14T13:01:25.615009Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation eb3817d8-a000-496f-aad8-b6c99cff40ea · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 41
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.619191Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a73a9c67-d10f-40c1-9028-c7d5cf45292e · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 42
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.622828Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d896d9fb-fa33-4415-aecf-2ae6c9ea4f5c · outbound
This paper cites 2013a, A&A, 558, A131.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2013a, A&A, 558, A131
Reference 43
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.626511Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 72f56cf4-fb7d-4d7d-9af2-0c79f0d8f2bf · outbound
This paper cites 2013b, A&A, 550, L7.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2013b, A&A, 550, L7
Reference 44
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.629833Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation e26ea30e-1cb6-4475-ad72-212ba46fa761 · outbound
This paper cites 2009, AJ, 138, 1243.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2009, AJ, 138, 1243
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.632778Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 475ba7d3-3ca2-43b6-91cd-7a000b7194cb · outbound
This paper cites L., Woosley S.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars L., Woosley S
Reference 46
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T13:01:25.635856Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cc56537d-3e8a-43bd-9684-4f5f11f584ce · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 47
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.856863Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation c0e84d27-68d7-415a-adaa-ec0cc533f69d · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 48
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.845892Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation dfa444a0-f5e4-473a-af36-fce52613a342 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 49
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.834122Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 61d1d3f8-8370-4764-a10a-45fd169f415c · outbound
This paper cites 2016, ApJ, 825, 64.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2016, ApJ, 825, 64
Reference 50
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.822617Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation ce750395-f19f-4fb3-b875-e0822ca2a83d · outbound
This paper cites 2014, ApJ, 796, 121.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2014, ApJ, 796, 121
Reference 51
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.811796Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation bf17abae-d2d3-477a-a651-3bdc1f15c9bf · outbound
This paper cites 2012, ApJ, 759, 107.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2012, ApJ, 759, 107
Reference 52
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.802054Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation c3a83456-c819-40d8-b16e-7eadb1182cc2 · outbound
This paper cites 2016, ApJ, 831, 205.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2016, ApJ, 831, 205
Reference 53
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.792413Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 8e4965f2-da10-4ced-bb78-b2685824b182 · outbound
This paper cites 2018, Nature Astronomy, 2, 334.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2018, Nature Astronomy, 2, 334
Reference 54
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.782203Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation c6f0aa3f-3718-43b7-ad56-f09943cc98f4 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 55
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.771161Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 474d8b75-7f93-4f2b-9fb1-b70200f885b9 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 56
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.761297Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 8cb77062-9843-4558-ba23-2aafaad00308 · outbound
This paper cites 2000, Ph.
Reference 57
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.750533Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 2e6f4581-2211-403e-b0a5-693bd3b348cd · outbound
This paper cites S.\ 2006,.
Reference 58
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.738879Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 8aefdb79-0031-4c47-a1e0-a5138583810c · outbound
This paper cites 1994, A&A, 290, 819.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1994, A&A, 290, 819
Reference 59
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.728784Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 085485d1-4cf1-46bd-95c6-a7734491fe25 · outbound
This paper cites 1989, in Physics of Luminous Blue Variables, ed.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1989, in Physics of Luminous Blue Variables, ed
Reference 60
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.718842Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation e2e99845-172d-495a-b22b-0f49315fa621 · outbound
This paper cites 1974, ApJS, 255, 28.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1974, ApJS, 255, 28
Reference 61
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.708863Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f3a5b7d2-a208-4c8c-bb0e-0098c3a2643d · outbound
This paper cites 1980, AJ, 85, 1046.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1980, AJ, 85, 1046
Reference 62
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.698603Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 5448a262-770e-4992-b9ea-253d698dc20f · outbound
This paper cites 1989, in Physics of Luminous Blue Variables, ed.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1989, in Physics of Luminous Blue Variables, ed
Reference 63
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.688250Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 8f98b4b5-bdc7-46a4-b612-209b467ffac0 · outbound
This paper cites 2002, A&A, 382, 999.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2002, A&A, 382, 999
Reference 64
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.676425Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation f1b0994b-f850-4b76-b202-09ef11b3a76d · outbound
This paper cites 1995, ApJ, 438, 188.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1995, ApJ, 438, 188
Reference 65
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.666022Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 1c0a4f47-3546-40b5-9844-f022c997d003 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 66
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.655993Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation e7fd1b00-aed4-4882-90a3-bc7ecd91ada5 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 67
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.645468Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 64f4f6ab-c03b-47fe-9e50-b2c1df7c6f83 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 68
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.636039Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 2b83f32d-047c-4a2d-9f3a-dcb10c6f7909 · outbound
This paper cites 2017, MNRAS, 469, 4649.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2017, MNRAS, 469, 4649
Reference 69
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.626150Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 490d1fa6-79f3-4a4b-9286-bda5164d0c2f · outbound
This paper cites 2003, A&A, 404,975.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2003, A&A, 404,975
Reference 70
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.614975Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 36b84062-438f-4088-b238-24ed06b88cbc · outbound
This paper cites 2011, Bull.\ Soc.\ R.\ Sci.\ Lie'ge, 80, 266.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2011, Bull.\ Soc.\ R.\ Sci.\ Lie'ge, 80, 266
Reference 71
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.604719Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 705898a5-3e34-4e21-902a-a1a8063394f7 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 72
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.593317Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 84f116e2-6f4c-4c3a-9919-755a4f113f02 · outbound
This paper cites 2018, ApJ, 863, 181.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2018, ApJ, 863, 181
Reference 73
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.580751Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation bd84f440-95ca-4514-a1d3-94dbc2b2a26f · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 74
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.570363Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 5cf089c7-3f9e-4597-8139-d6ac7b62651e · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 75
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.559317Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 41dc70fd-2fa3-4681-8820-cadd84a1a76d · outbound
This paper cites 2016, A&A, 590,.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2016, A&A, 590,
Reference 76
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.547904Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 2f67ea02-17ac-4266-84d4-e9474f4c6a99 · outbound
This paper cites 2005, in The Fate of the.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2005, in The Fate of the
Reference 77
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.537198Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation ae3febaf-84ae-40f2-bfbb-81c356dafb89 · outbound
This paper cites 1997, in.
Reference 78
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.525740Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation bfa9ae51-1c13-4ddd-9409-d7db0cba9a44 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 79
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.515564Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 71793bf0-27d5-4e56-ad7a-d5e12979b97b · outbound
This paper cites 2004, ApJ, 616, 525.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2004, ApJ, 616, 525
Reference 80
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.503967Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 9329384f-b767-4162-b7f0-27d9458b972b · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 81
- Resolution
- parse uncertain
- raw_fallback, observed 2026-08-14T13:01:26.492362Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation fd80b99e-7613-4092-ba8d-c7e4996af63a · outbound
This paper cites 1961, Acta Astron., 17, 355.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1961, Acta Astron., 17, 355
Reference 82
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.481689Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 8254a9f5-e41b-4f0c-8fb8-379d5a1b3bb2 · outbound
This paper cites 2010, New Astron.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2010, New Astron
Reference 83
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.470817Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation a0777d09-5035-4bce-b83c-dab89ed9bcd1 · outbound
This paper cites 1992, ApJ, 391, 246.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1992, ApJ, 391, 246
Reference 84
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.460823Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 4b92eb83-a20d-4126-9c41-b59bdc122d52 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 85
- Resolution
- parse uncertain
- raw_fallback, observed 2026-08-14T13:01:26.451136Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 0637dacb-dff3-4991-879b-57b6fe43edcf · outbound
This paper cites 1967, MNRAS, 135, 251.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 1967, MNRAS, 135, 251
Reference 86
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.441020Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 34e4aa11-2166-44ab-b5f7-bc8e0ed1168e · outbound
This paper cites 2019, A&A, 624, A66.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2019, A&A, 624, A66
Reference 87
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.430306Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation dbe03554-8c4a-4327-9ed1-bcd25d245f1f · outbound
This paper cites 2012, Science, 337, 444.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2012, Science, 337, 444
Reference 88
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.419230Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 4c17e0e0-fb66-4d16-8c56-98c3e0e9d443 · outbound
This paper cites 2014, ApJ, 780, 117.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2014, ApJ, 780, 117
Reference 89
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.408943Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation e98a1408-8c73-4fda-9bac-3e05551e1cfa · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 90
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.398489Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation edb191ad-5114-4374-b94a-367b44f4a108 · outbound
This paper cites 2011, in Active OB Stars:.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2011, in Active OB Stars:
Reference 91
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.388835Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation a766e1d1-b64a-4e9b-86dd-cf73b3c81cce · outbound
This paper cites 2014, ARAA, 52, 487.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2014, ARAA, 52, 487
Reference 92
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.377012Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 5153b8eb-3231-4e93-a826-acbc203909e3 · outbound
This paper cites 2016, MNRAS, 461, 3353.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2016, MNRAS, 461, 3353
Reference 93
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.366299Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 251cbe44-d9f7-4d1f-8ab9-c42d0caee063 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 94
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.355817Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation a380d3ae-49da-44fc-a2ee-d38b61e3ca94 · outbound
This paper cites 2008, ApJ, 679, 1467.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2008, ApJ, 679, 1467
Reference 95
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.346031Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation fae32d19-8590-49cd-bbc8-e94bea9d8ab9 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 96
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.335522Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation 9376cfc0-2ed6-423a-bdda-41455b194817 · outbound
This paper cites 2006, ApJ, 645, L45.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2006, ApJ, 645, L45
Reference 97
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.323913Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation ad664d24-1e47-4014-8e4f-b94c5532b3f9 · outbound
This paper cites 2015, MNRAS, 447, 602.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars 2015, MNRAS, 447, 602
Reference 98
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-14T13:01:26.314696Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation db4f7201-8e7f-40a2-a788-a8f48c2a9aba · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 99
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.304074Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Observation b5b855c9-1c3f-41b3-b9d9-8c2d3f0e4247 · outbound
This paper cites an unresolved cited work.
The isolation of Luminous Blue Variables resembles aging B-type supergiants, not the most massive unevolved stars Unresolved cited work
Reference 100
- Resolution
- unresolved
- raw_fallback, observed 2026-08-14T13:01:26.293807Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.
Pith citing papers
No inbound Pith citation observations are available.