Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation | Paper Citation Record

Observation 90e6f7e6-0866-484a-8b9c-c83bd770332a · outbound

This paper cites Their formation and evolution are still poorly understood (e.g., [1]).

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Their formation and evolution are still poorly understood (e.g., [1])

Reference 1

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Observation 7ae65433-0839-4887-b7d4-3c4370236e44 · outbound

This paper cites The list of sources is given in Table 1.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation The list of sources is given in Table 1

Reference 2

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.472873Z

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Observation 3e4b6461-be65-4a1f-9a77-8e7e9c2738c7 · outbound

This paper cites The spectra were fitted with Gaussian profiles using theLMFIT package [24].

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation The spectra were fitted with Gaussian profiles using theLMFIT package [24]

Reference 3

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.455291Z

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Observation ec0c5ca6-770b-47ba-b83e-370d35808ce2 · outbound

This paper cites Clumps identification from dust emission To extract the clumps, we use Python Astrodendro4 [26].

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Clumps identification from dust emission To extract the clumps, we use Python Astrodendro4 [26]

Reference 4

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Observation a64bd801-bb18-43af-a89f-63d5a6c62499 · outbound

This paper cites 2" and "3.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation 2" and "3

Reference 5

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.417879Z

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Observation 780eaa34-a3bf-4b90-bbfe-a6685643f5cd · outbound

This paper cites We observed HCN, HNC, HCO+, HC3N, HNCO, OCS, CS, SiO, SO2, and SO lines with the IRAM-30m radio telescope.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation We observed HCN, HNC, HCO+, HC3N, HNCO, OCS, CS, SiO, SO2, and SO lines with the IRAM-30m radio telescope

Reference 6

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Observation 3eef9433-5de1-4d6c-b065-c43a969ca679 · outbound

This paper cites Three clumps were found to be associated with the Hii regions, 10 with YSOs, and 7 with submillimetre emission.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Three clumps were found to be associated with the Hii regions, 10 with YSOs, and 7 with submillimetre emission

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.383618Z

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Observation cab3a2f9-b4c9-4559-b169-b14397dc5bd3 · outbound

This paper cites However, a strong correlation is observed in the mass–size relationships.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation However, a strong correlation is observed in the mass–size relationships

Reference 8

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.364770Z

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Observation 7db63d2f-e09d-4a16-b481-298372a4e9d3 · outbound

This paper cites The average line widths are about 3 kms−1, with a minimum for C34S (2.4 kms −1) and a maximum for SiO (5.5 kms−1).

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation The average line widths are about 3 kms−1, with a minimum for C34S (2.4 kms −1) and a maximum for SiO (5.5 kms−1)

Reference 9

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.345986Z

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Observation 27ff97de-6bb4-467e-b5cd-b202e1f8add3 · outbound

This paper cites High-Mass Star and Massive Cluster Formation in the Milky Way.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation High-Mass Star and Massive Cluster Formation in the Milky Way

Reference 10

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Observation 951e0d06-e506-495a-9b05-d90c6af552c8 · outbound

This paper cites Toward Understanding Massive Star Formation.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Toward Understanding Massive Star Formation

Reference 11

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Observation 758767d6-8679-4416-9d93-134c7ad898a7 · outbound

This paper cites an unresolved cited work.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Unresolved cited work

Reference 12

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Observation f66fc0a6-73ac-4904-b2ee-6a5cb3e908f4 · outbound

This paper cites an unresolved cited work.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Unresolved cited work

Reference 13

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Observation 9789a5b9-da55-4d2a-86a8-cde1da6ecb25 · outbound

This paper cites an unresolved cited work.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Unresolved cited work

Reference 14

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:45:24.292953Z

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Observation 6fc217c1-9487-4958-862e-815cf14aab56 · outbound

This paper cites Caselli and P.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Caselli and P

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.275859Z

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Observation 656fbe26-d9ff-4e13-9852-3668aabe6d81 · outbound

This paper cites an unresolved cited work.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Unresolved cited work

Reference 16

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:45:24.257729Z

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Observation 7864c625-d234-42a1-871c-c2294e1f2d21 · outbound

This paper cites The Universality of Turbulence in Galactic Molecular Clouds.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation The Universality of Turbulence in Galactic Molecular Clouds

Reference 17

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Observation 4d1427d6-4efe-4846-8990-ca829b154bf2 · outbound

This paper cites Testing Larson's relationships in massive clumps.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Testing Larson's relationships in massive clumps

Reference 18

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Observation 8364552c-e93a-4e3f-ba27-91642379eae4 · outbound

This paper cites Bertoldi and C.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Bertoldi and C

Reference 19

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.240375Z

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Observation 25b8e410-b3ed-4b70-aba7-c073b6ae7f4d · outbound

This paper cites Kauffmann, T.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Kauffmann, T

Reference 20

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.223354Z

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Observation d622258d-d6d3-4e76-93e6-e7c8c7c89f03 · outbound

This paper cites Magnetic Fields in High-Mass Infrared Dark Clouds.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Magnetic Fields in High-Mass Infrared Dark Clouds

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.751052Z

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Observation 96c4dfb7-335e-4d69-9282-ccc217af0c90 · outbound

This paper cites Chemistry in Infrared Dark Clouds.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Chemistry in Infrared Dark Clouds

Reference 22

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Observation 079f5beb-013e-4309-a40b-94c4cd2b7096 · outbound

This paper cites Chemistry in Infrared Dark Cloud Clumps: a Molecular Line Survey at 3 mm.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Chemistry in Infrared Dark Cloud Clumps: a Molecular Line Survey at 3 mm

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.761165Z

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Observation 6beb0634-13b9-4ade-8609-fa1b1827fc4f · outbound

This paper cites Chemical evolution in the early phases of massive star formation. I.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Chemical evolution in the early phases of massive star formation. I

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:45:23.819234Z

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Observation be4ba4bc-83eb-42b2-863f-71075b89480e · outbound

This paper cites an unresolved cited work.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Unresolved cited work

Reference 25

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:45:24.206187Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation d8f909e9-bc02-4b27-83c7-e570ac89ce4f · outbound

This paper cites ATLASGAL --- Molecular fingerprints of a sample of massive star forming clumps.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation ATLASGAL --- Molecular fingerprints of a sample of massive star forming clumps

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.776280Z

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Observation 7ef7892f-2162-4558-a0bb-5a56b315e7c9 · outbound

This paper cites H$^{13}$CN-HN$^{13}$C intensity ratio as a temperature indicator of interstellar clouds.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation H$^{13}$CN-HN$^{13}$C intensity ratio as a temperature indicator of interstellar clouds

Reference 27

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:45:23.776251Z

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Observation 7b358783-2b48-4ccb-8246-f04e475cfa41 · outbound

This paper cites an unresolved cited work.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Unresolved cited work

Reference 28

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:45:24.188765Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation fb8f6499-1b89-4452-a964-1e8ca8c09450 · outbound

This paper cites Di Francesco, D.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Di Francesco, D

Reference 29

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.172730Z

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Observation 5ee8859c-1756-435f-a796-5adf332ef003 · outbound

This paper cites The Red MSX Source Survey: the Massive Young Stellar Population of our Galaxy.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation The Red MSX Source Survey: the Massive Young Stellar Population of our Galaxy

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.798524Z

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Observation 86efa1fc-ce42-4385-add2-a7a061a0641f · outbound

This paper cites Sepúlveda, R.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Sepúlveda, R

Reference 31

Resolution: verified exact; arxiv_id, observed 2026-08-11T04:45:23.734159Z

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Observation a4a325e5-4d49-4ded-bcf6-8c3aa97dcfe7 · outbound

This paper cites an unresolved cited work.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Unresolved cited work

Reference 32

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:45:24.156990Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 0cbe6160-25a3-4054-8948-aa24fd4623ba · outbound

This paper cites Newville, T.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Newville, T

Reference 33

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.141293Z

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Observation aa331a6f-a973-41db-bcbb-087baa701b66 · outbound

This paper cites Dynamic star formation in the massive DR21 filament.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Dynamic star formation in the massive DR21 filament

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.819257Z

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Observation 6db20f4e-5d8e-4938-9d88-b85858576747 · outbound

This paper cites Structural Analysis of Molecular Clouds: Dendrograms.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Structural Analysis of Molecular Clouds: Dendrograms

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.824371Z

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Observation fe493347-e6eb-47d6-a85f-cc5d2a287c96 · outbound

This paper cites APEX/SABOCA observations of small-scale structure of infrared-dark clouds I. Early evolutionary stages of star-forming cores.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation APEX/SABOCA observations of small-scale structure of infrared-dark clouds I. Early evolutionary stages of star-forming cores

Reference 36

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:45:23.527877Z

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Observation 05de5852-66d6-4718-b89f-28aaa3053041 · outbound

This paper cites an unresolved cited work.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Unresolved cited work

Reference 37

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:45:24.123675Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 9a91c93a-ac2e-4400-9f64-ee259646b96c · outbound

This paper cites Kauffmann, F.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Kauffmann, F

Reference 38

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.101932Z

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Observation 63ab4981-77dc-4ff4-afe3-da2727c314ec · outbound

This paper cites Ossenkopf and T.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Ossenkopf and T

Reference 39

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.076802Z

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Observation 61c341a4-cb33-4e13-9bd3-10b16d99de4f · outbound

This paper cites Hirota, S.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Hirota, S

Reference 40

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.058395Z

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Observation af78b85a-b5ce-4fbb-a5a4-5f5b36cc687c · outbound

This paper cites Hacar, A.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Hacar, A

Reference 41

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.038590Z

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Observation 4221b437-e6a9-4626-a808-ac05223f964f · outbound

This paper cites How to Calculate Molecular Column Density.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation How to Calculate Molecular Column Density

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.859911Z

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Observation a579238f-4b2c-41a9-9bfc-c8b62e2d77aa · outbound

This paper cites pyspeckit: A spectroscopic analysis and plotting package.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation pyspeckit: A spectroscopic analysis and plotting package

Reference 43

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:45:23.487441Z

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Observation 56234465-ba79-46ba-8b8b-091f5dedbc8c · outbound

This paper cites Direct measurements of carbon and sulfur isotope ratios in the Milky Way.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Direct measurements of carbon and sulfur isotope ratios in the Milky Way

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.869878Z

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Observation a9d37208-d715-46fb-9904-95452952b1c0 · outbound

This paper cites N2H+(1-0) survey of massive molecular cloud cores.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation N2H+(1-0) survey of massive molecular cloud cores

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:45:23.447092Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 5031b4f2-3ef1-4872-b3ce-be81d6d8ce97 · outbound

This paper cites an unresolved cited work.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Unresolved cited work

Reference 46

Resolution: unresolved; raw_fallback, observed 2026-08-11T04:45:24.021509Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation fcfbce82-919f-4f40-a2a2-a05b27b9d6c4 · outbound

This paper cites Are massive dense clumps truly sub-virial? A new analysis using Gould Belt ammonia data.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Are massive dense clumps truly sub-virial? A new analysis using Gould Belt ammonia data

Reference 47

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:45:23.423230Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation cb521244-3147-4d1e-bd57-5967dfbaab6c · outbound

This paper cites How Many Infrared Dark Clouds can form Massive Stars and Clusters?.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation How Many Infrared Dark Clouds can form Massive Stars and Clusters?

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.890533Z

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Observation fc652465-8f78-44cd-bf85-0ae707f71763 · outbound

This paper cites Chemical evolution of Red MSX Sources in the southern sky.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Chemical evolution of Red MSX Sources in the southern sky

Reference 49

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:45:23.379778Z

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No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 0aecf4e4-0a7b-4f0e-8a21-2a1d569d19b0 · outbound

This paper cites The SIMBAD astronomical database.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation The SIMBAD astronomical database

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.901196Z

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Observation 2d193a8f-fa48-4fed-94d5-8592c65d45e1 · outbound

This paper cites Ochsenbein, The vizier database of astronomical catalogues (1996), URL https://vizier.cds.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Ochsenbein, The vizier database of astronomical catalogues (1996), URL https://vizier.cds

Reference 51

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:24.004899Z

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Observation 78e040ac-3129-4dfc-a212-ca033044f886 · outbound

This paper cites Ochsenbein, P.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Ochsenbein, P

Reference 52

Resolution: verified exact; raw_fallback, observed 2026-08-11T04:45:23.339763Z

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Observation b65de3ce-38b7-4bbc-91a3-5411694a46eb · outbound

This paper cites Array Programming with NumPy.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Array Programming with NumPy

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.916157Z

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Unavailable: canonical work link unavailable.

Observation d13a846c-f671-4770-84f5-89f2a60b98f3 · outbound

This paper cites The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.921299Z

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Unavailable: canonical work link unavailable.

Observation d2f6c132-f9bf-4c2b-8455-295c8e5b73e0 · outbound

This paper cites an unresolved cited work.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Unresolved cited work

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.926583Z

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Unavailable: canonical work link unavailable.

Observation 6859ee81-ec16-4d27-90e7-589c09c26a6d · outbound

This paper cites SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation SciPy 1.0--Fundamental Algorithms for Scientific Computing in Python

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.931417Z

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Unavailable: canonical work link unavailable.

Observation 1d44544e-53d8-40e6-940c-77d1d422d86d · outbound

This paper cites Trigonometric Parallaxes of 6.7 GHz Methanol Masers.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Trigonometric Parallaxes of 6.7 GHz Methanol Masers

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.936578Z

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Unavailable: canonical work link unavailable.

Observation da95705c-2e00-4e79-a2cf-817515c7cfb8 · outbound

This paper cites Russeil, C.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Russeil, C

Reference 58

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:23.977895Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation fa97e37d-a363-4462-a8f3-cc22cf0d698b · outbound

This paper cites A `Water Spout' Maser Jet in S235AB-MIR.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation A `Water Spout' Maser Jet in S235AB-MIR

Reference 59

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:45:23.079154Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 74054fc9-6932-4184-8dcb-497eb0e92b5b · outbound

This paper cites Parallaxes and proper motions of interstellar masers toward the Cygnus X star-forming complex. I. Membership of the Cygnus X region.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Parallaxes and proper motions of interstellar masers toward the Cygnus X star-forming complex. I. Membership of the Cygnus X region

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-11T04:45:22.954603Z

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Unavailable: canonical work link unavailable.

Observation e24412c0-f88d-4a4e-93eb-fb8ed54d28a6 · outbound

This paper cites Trigonometric Parallaxes of Massive Star Forming Regions: II. Cep A & NGC 7538.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Trigonometric Parallaxes of Massive Star Forming Regions: II. Cep A & NGC 7538

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-08-11T04:45:23.037949Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation a24ea30b-3cf2-4d84-8898-74a2b4a9ab0e · outbound

This paper cites Zavagno, L.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation Zavagno, L

Reference 62

Resolution: verified fuzzy; raw_fallback, observed 2026-08-11T04:45:23.961651Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

Observation 4e7480dc-8200-46c7-8855-e1604181f810 · outbound

This paper cites The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance.

Study of the physical and chemical properties of dense clumps at different evolutionary stages in several regions of massive star and stellar cluster formation The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance

Reference 63

Resolution: malformed identifier; no resolver link, observed 2026-08-11T04:45:22.970126Z

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Unavailable: canonical work link unavailable.

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