How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching | Paper Citation Record

Observation ad007e39-fd10-4d98-b286-992991f03ffe · outbound

This paper cites Testing the bloated star hypothesis in the massive young stellar object IRAS 19520+2759 through optical and infrared variability.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Testing the bloated star hypothesis in the massive young stellar object IRAS 19520+2759 through optical and infrared variability

Reference 1

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Observation 47c551ef-0ad0-45e0-b9cf-58ada9764d2b · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 2

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Observation 75bfd183-c25d-4f10-a98d-036e9e713ac1 · outbound

This paper cites Thermal Jeans fragmentation within 1000 AU in OMC-1S.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Thermal Jeans fragmentation within 1000 AU in OMC-1S

Reference 3

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Observation 3e24000f-5a1d-41a7-896f-58a5147c2053 · outbound

This paper cites , year = 1955, month = jan, volume =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , year = 1955, month = jan, volume =

Reference 4

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Observation 2152c172-3974-4881-88ef-808175c738a2 · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:56.575042Z

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Observation 60704e6e-1463-46c4-8042-d7f541e3b43d · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 6

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Observation 30a9bf20-5c3a-4590-b60a-50931cc6921f · outbound

This paper cites The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The Initial Mass Function of Stars: Evidence for Uniformity in Variable Systems

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:56.845631Z

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Observation 4e9bfd71-586e-4f4a-b8cf-6d349f7d2941 · outbound

This paper cites Galactic Stellar and Substellar Initial Mass Function.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Galactic Stellar and Substellar Initial Mass Function

Reference 8

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Observation a1bbee5e-e830-44d7-958b-2fac30589bc8 · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:57.128841Z

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Observation 6a7b8a02-70a4-4cf2-a532-e79b2f7e4cb3 · outbound

This paper cites Star formation in clusters: a survey of compact mm-wave sources in the Serpens core.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Star formation in clusters: a survey of compact mm-wave sources in the Serpens core

Reference 10

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Observation 69388ca5-6f6d-4467-be31-59f54ed413e8 · outbound

This paper cites The mass function of dense molecular cores and the origin of the IMF.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The mass function of dense molecular cores and the origin of the IMF

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:57.429787Z

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Observation 9ad858e0-f9a4-42d8-b5d7-6d0b516e4f3e · outbound

This paper cites From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching From filamentary clouds to prestellar cores to the stellar IMF: Initial highlights from the Herschel Gould Belt survey

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:57.597656Z

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Observation c871f1d4-74eb-4056-bfdd-aaf1079087e7 · outbound

This paper cites Star Formation in Galaxies Along the Hubble Sequence.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Star Formation in Galaxies Along the Hubble Sequence

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:57.760755Z

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Observation 487f5b05-0301-4867-a4ef-fa0f35019696 · outbound

This paper cites A Universal Stellar Initial Mass Function? A Critical Look at Variations.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching A Universal Stellar Initial Mass Function? A Critical Look at Variations

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:57.887071Z

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Observation a6f3fe85-d866-4b47-9338-4c668bb43dbe · outbound

This paper cites The Origin and Universality of the Stellar Initial Mass Function.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The Origin and Universality of the Stellar Initial Mass Function

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:58.037837Z

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Observation 7efea67f-fdcc-4210-bc4a-39a96f2d1618 · outbound

This paper cites Frontiers in Astronomy and Space Sciences , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Frontiers in Astronomy and Space Sciences , keywords =

Reference 16

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Observation 1f07f07e-8d1d-4fcd-bd2f-621deb471e64 · outbound

This paper cites What is the role of stellar radiative feedback in setting the stellar mass spectrum?.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching What is the role of stellar radiative feedback in setting the stellar mass spectrum?

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:58.368224Z

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Observation 739bb1d7-eab8-4c7a-84f5-70a40924bcb9 · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:58.484561Z

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Observation ca21fc16-ec41-43dd-bca4-8e3c31e73327 · outbound

This paper cites Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:58.643897Z

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Observation 4580c04d-5700-4d7a-97e0-653fc731e2e9 · outbound

This paper cites A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching A census of dense cores in the Aquila cloud complex: SPIRE/PACS observations from the Herschel Gould Belt survey

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:58.775095Z

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Observation 347fdbf3-dd8c-476f-9ad5-1d580a39a8bf · outbound

This paper cites Star formation from low to high mass: A comparative view.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Star formation from low to high mass: A comparative view

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:58.840762Z

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Observation ab3be1b7-765b-4e92-9e22-85c6725159e6 · outbound

This paper cites Disentangling the independently controllable factors of variation by interacting with the world.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Disentangling the independently controllable factors of variation by interacting with the world

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:58.984137Z

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Observation 0da8f5a6-8d77-4871-83dc-d9e9ddfe88fa · outbound

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

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching High-Mass Star and Massive Cluster Formation in the Milky Way

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:59.106947Z

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Observation 0c85bfbe-c6c6-4472-a807-7ba30cee5cf7 · outbound

This paper cites On the totally positive grassmannian.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching On the totally positive grassmannian

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:59.220123Z

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Observation e5184e8f-7187-46f7-83e9-df14b2fc3d5e · outbound

This paper cites ALMA-IMF XV: The core mass function in the high-mass star-formation regime.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF XV: The core mass function in the high-mass star-formation regime

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:59.344893Z

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Observation c6eee11e-bfc5-4fe1-b3e1-e9d567cb08d9 · outbound

This paper cites The fragmentation properties of massive star-forming regions in 30Dor-10 at 2000 au resolution.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The fragmentation properties of massive star-forming regions in 30Dor-10 at 2000 au resolution

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:59.482720Z

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Observation 443cc020-9d15-4ace-bdf4-cfecc1f33501 · outbound

This paper cites ALMA-IMF I -- Investigating the origin of stellar masses: Introduction to the Large Program and first results.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF I -- Investigating the origin of stellar masses: Introduction to the Large Program and first results

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:59.634722Z

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Observation d001e24e-8cc9-467a-a090-793933824294 · outbound

This paper cites ALMAGAL I. The ALMA evolutionary study of high-mass protocluster formation in the Galaxy. Presentation of the survey and early results.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMAGAL I. The ALMA evolutionary study of high-mass protocluster formation in the Galaxy. Presentation of the survey and early results

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:59.774176Z

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Observation 4add9564-bc07-4ead-87e6-2a34ece0eca9 · outbound

This paper cites ALMAGAL III. Compact source catalog: Fragmentation statistics and physical evolution of the core population.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMAGAL III. Compact source catalog: Fragmentation statistics and physical evolution of the core population

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:59.889481Z

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Observation 78b05cf7-bc3e-41aa-bf1a-cbc2d7f3a932 · outbound

This paper cites Linear filament and nested cluster evolution tomography (LANCET) I. Capture the evolution of dense gas in 14-parsec filament G316.8.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Linear filament and nested cluster evolution tomography (LANCET) I. Capture the evolution of dense gas in 14-parsec filament G316.8

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-02T07:31:59.976850Z

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Observation 83e7dc45-eefb-43b7-a498-39db62f29a1d · outbound

This paper cites The ALMA-QUARKS Survey: II. the ACA 1.3 mm continuum source catalog and the assembly of dense gas in massive star-forming clumps.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The ALMA-QUARKS Survey: II. the ACA 1.3 mm continuum source catalog and the assembly of dense gas in massive star-forming clumps

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:00.091804Z

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Observation 3966f5ef-1fdf-4fa5-831d-53d3f454f955 · outbound

This paper cites The ALMA-QUARKS survey: -- I. Survey description and data reduction.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The ALMA-QUARKS survey: -- I. Survey description and data reduction

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:00.224464Z

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Observation 9bf641e6-c90f-41e1-8480-d6a877accb1a · outbound

This paper cites an unresolved cited work.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Unresolved cited work

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:00.328712Z

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Observation a363862b-7a5c-4d94-899f-4cd846b8a8fe · outbound

This paper cites The ALMA Survey of 70 $\mu$m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The ALMA Survey of 70 $\mu$m dark High-mass clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:00.450404Z

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Observation 4063e6e9-a91c-48d8-bc3a-594cc5969b06 · outbound

This paper cites The ALMA Survey of 70 $\mu$m Dark High-mass Clumps in Early Stages (ASHES). IX. Physical Properties and Spatial Distribution of Cores in IRDCs.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The ALMA Survey of 70 $\mu$m Dark High-mass Clumps in Early Stages (ASHES). IX. Physical Properties and Spatial Distribution of Cores in IRDCs

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:00.637870Z

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Observation dd2f5880-383e-4043-82c3-5345fdc74777 · outbound

This paper cites The ALMA Survey of 70 $\mu$m Dark High-mass Clumps in Early Stages (ASHES). XI. Statistical Study of Early Fragmentation.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The ALMA Survey of 70 $\mu$m Dark High-mass Clumps in Early Stages (ASHES). XI. Statistical Study of Early Fragmentation

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:00.726297Z

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Observation 7e5f1fd8-aeae-468d-9073-4ecc2ba77c68 · outbound

This paper cites Dual-band Unified Exploration of Three CMZ Clouds (DUET). Cloud-wide census of continuum sources showing low spectral indices.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Dual-band Unified Exploration of Three CMZ Clouds (DUET). Cloud-wide census of continuum sources showing low spectral indices

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:00.866296Z

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Observation 2cdd0789-9fb2-4c83-87f1-fdcc41eebeaa · outbound

This paper cites ALMA Observations of Massive Clouds in the Central Molecular Zone: External-Pressure-Confined Dense Cores and Salpeter-like Core Mass Functions.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA Observations of Massive Clouds in the Central Molecular Zone: External-Pressure-Confined Dense Cores and Salpeter-like Core Mass Functions

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:00.983615Z

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Observation e30f1333-247f-41ac-bdbf-c19c5b9a3a99 · outbound

This paper cites ALMA Observations of Massive Clouds in the Central Molecular Zone: Jeans Fragmentation and Cluster Formation.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA Observations of Massive Clouds in the Central Molecular Zone: Jeans Fragmentation and Cluster Formation

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:01.175711Z

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Observation 9350b7a6-02bb-4d8e-bafe-b19df814c66f · outbound

This paper cites Star Formation in the Central Molecular Zone of the Milky Way.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Star Formation in the Central Molecular Zone of the Milky Way

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:01.355260Z

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Observation 26549cfc-dd15-45d1-bc1b-4c5b3fdfe8d6 · outbound

This paper cites Stellar initial mass function in the 100-pc solar neighbourhood.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Stellar initial mass function in the 100-pc solar neighbourhood

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:01.503737Z

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Observation e6bc853e-dac7-48b0-8d42-b221d0124e3b · outbound

This paper cites Power-law distributions in empirical data.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Power-law distributions in empirical data

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:01.714322Z

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Observation 1f44cc92-3f74-4d41-aa8e-21c73da2332e · outbound

This paper cites Does God play dice with star clusters?.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Does God play dice with star clusters?

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:01.841902Z

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Observation 73b1bd5c-2608-45de-825c-deb78082561e · outbound

This paper cites ALMA-IMF III -- Investigating the origin of stellar masses: Top-heavy core mass function in the W43-MM2&MM3 mini-starburst.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF III -- Investigating the origin of stellar masses: Top-heavy core mass function in the W43-MM2&MM3 mini-starburst

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:01.932530Z

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Observation dec4a485-750c-437e-b714-ecf2d67e785b · outbound

This paper cites ALMA-IMF XXII. Role of core subfragmentation in the IMF origin: Hierarchical fragmentation cascade and CMF in W43-MM1.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF XXII. Role of core subfragmentation in the IMF origin: Hierarchical fragmentation cascade and CMF in W43-MM1

Reference 45

Resolution: verified exact; local_arxiv, observed 2026-08-02T07:33:28.122949Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation b34ba670-a4b7-4961-a8d9-0a1a5b91125c · outbound

This paper cites ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF. XXI.: N$_2$H$^+$ kinematics in the G012.80 protocluster: Evidence for filament rotation and evolution

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-08-02T07:33:27.885451Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 00ebce07-16fb-4b66-9e57-1c92b380acf0 · outbound

This paper cites ALMA-IMF XIII: N$_2$H$^+$ kinematic analysis on the intermediate protocluster G353.41.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF XIII: N$_2$H$^+$ kinematic analysis on the intermediate protocluster G353.41

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:02.418963Z

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Observation 14d18c73-b51b-486e-a947-a67dc1a1181d · outbound

This paper cites ALMA-IMF XVIII: The assembly of a star cluster: Dense N$_2$H$^+$ (1-0) kinematics in the massive G351.77 protocluster.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF XVIII: The assembly of a star cluster: Dense N$_2$H$^+$ (1-0) kinematics in the massive G351.77 protocluster

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:02.574352Z

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Observation 793a63e9-ee59-41cf-b9af-33cbd6ea46e7 · outbound

This paper cites A protostellar system fed by a streamer of 10,500 au length.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching A protostellar system fed by a streamer of 10,500 au length

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:02.671277Z

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Observation 8cb1439a-4264-4468-96bd-e3c824f1d538 · outbound

This paper cites Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Dynamical Accretion Flows -- ALMAGAL: Flows along filamentary structures in high-mass star-forming clusters

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:02.801844Z

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Observation 01b41144-a32f-4c4e-b6bf-2a6202857b59 · outbound

This paper cites Accelerating star formation of dense clumps.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Accelerating star formation of dense clumps

Reference 51

Resolution: metadata mismatch; local_arxiv, observed 2026-08-02T07:33:27.654619Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 50270c85-59bd-4db6-8e84-9cd2a2af65e3 · outbound

This paper cites A graph theory-based multi-scale analysis of hierarchical cascade in molecular clouds : Application to the NGC 2264 region.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching A graph theory-based multi-scale analysis of hierarchical cascade in molecular clouds : Application to the NGC 2264 region

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:03.123787Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4956a810-8d7e-45e4-b199-8dd4930e470b · outbound

This paper cites The Origin and Evolution of Multiple Star Systems.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The Origin and Evolution of Multiple Star Systems

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:03.270467Z

Source-reported events for the cited work

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Observation 86a84d6d-3bce-457e-b146-52cb7efa34a4 · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:03.371501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 93e8eccc-ac9c-4e3a-a9e6-885dd09e4079 · outbound

This paper cites ALMA-IMF XII: Point-process mapping of 15 massive protoclusters.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF XII: Point-process mapping of 15 massive protoclusters

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:03.452629Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1f49d93c-f720-43de-a8cf-f66e49c2fc1f · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:03.576766Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0339a4cc-0595-4fde-a579-04242be32d66 · outbound

This paper cites an unresolved cited work.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Unresolved cited work

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:03.632928Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation facb96a3-2073-47ea-a0e7-66c1cc8a4093 · outbound

This paper cites Observations of high-order multiplicity in a high-mass stellar protocluster.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Observations of high-order multiplicity in a high-mass stellar protocluster

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:03.704292Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2e4b24be-009a-409b-b9eb-7d4814fb4991 · outbound

This paper cites ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XV. Steady Accretion from Global Collapse to Core Feeding in Massive Hub-filament System SDC335.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ATOMS: ALMA Three-millimeter Observations of Massive Star-forming regions -- XV. Steady Accretion from Global Collapse to Core Feeding in Massive Hub-filament System SDC335

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:03.767283Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6e8bd23-9b77-4ab4-8929-b2af1cc27e5f · outbound

This paper cites The spatial distribution of dense cores during the evolution of cluster-forming massive clumps.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The spatial distribution of dense cores during the evolution of cluster-forming massive clumps

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:03.866383Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 44c7b444-f001-413a-9308-9af0b7a0fe8f · outbound

This paper cites Relations between the core populations and the parent clump physical properties.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Relations between the core populations and the parent clump physical properties

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:03.944410Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4b0d7b7e-1233-49c9-a7c4-6b30e8a71801 · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 62

Resolution: verified exact; doi, observed 2026-08-02T07:33:27.522493Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 4cf8c0ed-04ce-4fc2-a92b-d4dc1273c3a7 · outbound

This paper cites ALMA-IMF. V. Prestellar and protostellar core populations in the W43 cloud complex.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF. V. Prestellar and protostellar core populations in the W43 cloud complex

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:04.050737Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation abfbdab7-06b5-418b-9e14-5936df909589 · outbound

This paper cites an unresolved cited work.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Unresolved cited work

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:04.192436Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3177c4fb-91c6-4f66-bdce-7a45a14cf693 · outbound

This paper cites The Rosetta Stone project. III. ALMA synthetic observations of fragmentation in high-mass star-forming clumps.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The Rosetta Stone project. III. ALMA synthetic observations of fragmentation in high-mass star-forming clumps

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:04.342355Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 790449a9-3ac3-4424-8bf7-ec003f93dfc7 · outbound

This paper cites The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The Rosetta Stone Project. II. The correlation between star formation efficiency and L/M indicator for the evolutionary stages of star-forming clumps in post-processed radiative magnetohydrodynamics simulations

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:04.538630Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6f6962a6-426a-491e-af3e-131b7f15b5dd · outbound

This paper cites The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The Rosetta Stone Project. I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:04.668659Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d2897e04-7a9a-4355-9cce-9eaf2a3a613c · outbound

This paper cites 2026 , eprint=.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching 2026 , eprint=

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:04.742303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation deeec0f9-c232-4c7e-a597-a5cee589b2b5 · outbound

This paper cites Fragmentation in Massive Star Formation.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Fragmentation in Massive Star Formation

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:04.795396Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 05ed3e2d-8593-4506-9a80-f6460a0eebe0 · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:04.970894Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 956dd8f0-958c-47fb-a2e5-b667ff7ce9ac · outbound

This paper cites Core mass function of a single giant molecular cloud complex with ~10^4 cores.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Core mass function of a single giant molecular cloud complex with ~10^4 cores

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:05.118750Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eeeb1f71-ee87-40c5-9845-118f804923cf · outbound

This paper cites The ALMA Survey of 70 \mu m Dark High-mass Clumps in Early Stages (ASHES). VIII. Dynamics of Embedded Dense Cores.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The ALMA Survey of 70 \mu m Dark High-mass Clumps in Early Stages (ASHES). VIII. Dynamics of Embedded Dense Cores

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:05.239776Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f1f14aee-b2dd-4f90-8831-59862f5ff25f · outbound

This paper cites Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 $\mu$m Dark Massive Clumps.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Global and Local Infall in the ASHES Sample (GLASHES). II. Asymmetric Line Profiles around Dense Cores in 70 $\mu$m Dark Massive Clumps

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:05.346489Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fbc8f741-d813-4062-a387-040a6962e4cd · outbound

This paper cites an unresolved cited work.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Unresolved cited work

Reference 74

Resolution: verified exact; arxiv_id, observed 2026-08-02T07:33:27.334580Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation cfce5074-1896-4c26-a3ca-50b77bcee928 · outbound

This paper cites The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO

Reference 75

Resolution: metadata mismatch; local_arxiv, observed 2026-08-02T07:33:27.187775Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 194676b7-0967-442a-8c91-bbc0b70e3eca · outbound

This paper cites Virial-based extraction of structures in numerical simulations: The vibes tool.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Virial-based extraction of structures in numerical simulations: The vibes tool

Reference 76

Resolution: metadata mismatch; local_arxiv, observed 2026-08-02T07:33:26.873365Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation f6064dfd-2852-40dd-9d0a-8c1e497b6cba · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:05.615093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3249ea90-e021-44dc-b7c2-15275a744bea · outbound

This paper cites Frontiers in Astronomy and Space Sciences , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Frontiers in Astronomy and Space Sciences , keywords =

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:05.812061Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 42a11785-613f-42ce-942d-5db4f30ea594 · outbound

This paper cites The ALMA-QUARKS Survey: III. Clump-to-core fragmentation and search for high-mass starless cores.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The ALMA-QUARKS Survey: III. Clump-to-core fragmentation and search for high-mass starless cores

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:05.953874Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c89c6b7b-e645-4cfe-80d5-c7f84b9c6a66 · outbound

This paper cites Core mass function in view of fractal and turbulent filaments and fibers.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Core mass function in view of fractal and turbulent filaments and fibers

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:06.048546Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 187bcf3b-29c6-4c94-9506-002e23ffe2e2 · outbound

This paper cites , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching , keywords =

Reference 81

Resolution: verified exact; doi, observed 2026-08-02T07:33:26.677445Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

Observation 80e5c681-2c40-4ceb-b3c2-6eaa5853121e · outbound

This paper cites ALMA-IMF XVI: Mass-averaged temperature of cores and protostellar luminosities in the ALMA-IMF protoclusters.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching ALMA-IMF XVI: Mass-averaged temperature of cores and protostellar luminosities in the ALMA-IMF protoclusters

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:06.411468Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 37c1e03a-1dc5-4c0e-b5fe-ae9cd69d312f · outbound

This paper cites Research in Astronomy and Astrophysics , keywords =.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching Research in Astronomy and Astrophysics , keywords =

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:06.590330Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6bf3d284-4e26-4a02-8937-86fcd61c79aa · outbound

This paper cites INvestigations of massive Filaments ANd sTar formation (INFANT). I. Core Identification and Core Mass Function.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching INvestigations of massive Filaments ANd sTar formation (INFANT). I. Core Identification and Core Mass Function

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:06.685278Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 65f00ccd-078d-41f4-adac-824c79d5e478 · outbound

This paper cites The Core Mass Function in the Massive Protocluster G286.21+0.17 revealed by ALMA.

How Should We Understand the Core Mass Function? A memo of the CMF2IMF conference at ESO Garching The Core Mass Function in the Massive Protocluster G286.21+0.17 revealed by ALMA

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-02T07:32:06.806232Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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