Emergence of high-mass stars in complex fiber networks (EMERGE): I. Early ALMA Survey: Observations and massive data reduction

A. Hacar; A. Socci; F. Bonanomi; D. Petry; M. Tafalla; D. Harsono; J. Forbrich; J. Alves; J. Grossschedl; J. R. Goicoechea; J. Pety; A. Burkert; G. X. Li

doi:10.1051/0004-6361/202348565

Emergence of high-mass stars in complex fiber networks (EMERGE): I. Early ALMA Survey: Observations and massive data reduction

A. Hacar, A. Socci, F. Bonanomi, D. Petry, M. Tafalla, D. Harsono, J. Forbrich, J. Alves, J. Grossschedl, J. R. Goicoechea, J. Pety, A. Burkert, G. X. Li

Research output: Contribution to journal › Article › peer-review

21 Downloads (Pure)

Abstract

(Abridged) Recent molecular surveys have revealed a rich gas organization of sonic-like fibers in all kind of environments prior to the formation of low- and high-mass stars. This paper introduces the EMERGE project aiming to investigate whether complex fiber arrangements could explain the origin of high-mass stars and clusters. We analyzed the EMERGE Early ALMA Survey including 7 star-forming regions in Orion (OMC-1/2/3/4 South, L1641N, NGC2023, and Flame Nebula) homogeneously surveyed in both molecular lines (N$_2$H$^+$ J=1-0, HNC J=1-0, plus HC3N J=10-9) and 3mm-continuum using a combination of interferometric ALMA mosaics and IRAM-30m single-dish (SD) maps. Based on our low-resolution (SD) observations, we describe the global properties of our sample covering a wide range of physical conditions including low-, intermediate, and high-mass star-forming regions in different evolutionary stages. Their comparison with ancillary YSO catalogs denotes N$_2$H$^+$ as the best proxy for the dense, star-forming gas in our targets showing a constant star formation efficiency and a fast time evolution of

Original language	English
Article number	A140
Pages (from-to)	1-37
Number of pages	37
Journal	Astronomy & Astrophysics
Volume	687
Early online date	5 Jul 2024
DOIs	https://doi.org/10.1051/0004-6361/202348565
Publication status	E-pub ahead of print - 5 Jul 2024

Keywords

astro-ph.GA
astro-ph.SR

Access to Document

10.1051/0004-6361/202348565Licence: CC BY

Final_Version
© 2024 The Author(s). Published by EDP Sciences, This is an open access article distributed under the terms of the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/
Final published version, 51.4 MBLicence: CC BY

Cite this

Hacar, A., Socci, A., Bonanomi, F., Petry, D., Tafalla, M., Harsono, D., Forbrich, J., Alves, J., Grossschedl, J., Goicoechea, J. R., Pety, J., Burkert, A., & Li, G. X. (2024). Emergence of high-mass stars in complex fiber networks (EMERGE): I. Early ALMA Survey: Observations and massive data reduction. Astronomy & Astrophysics, 687, 1-37. Article A140. Advance online publication. https://doi.org/10.1051/0004-6361/202348565

@article{9f420aef3db94562bc75bfe9a11409a5,

title = "Emergence of high-mass stars in complex fiber networks (EMERGE): I. Early ALMA Survey: Observations and massive data reduction",

abstract = "(Abridged) Recent molecular surveys have revealed a rich gas organization of sonic-like fibers in all kind of environments prior to the formation of low- and high-mass stars. This paper introduces the EMERGE project aiming to investigate whether complex fiber arrangements could explain the origin of high-mass stars and clusters. We analyzed the EMERGE Early ALMA Survey including 7 star-forming regions in Orion (OMC-1/2/3/4 South, L1641N, NGC2023, and Flame Nebula) homogeneously surveyed in both molecular lines (N$_2$H$^+$ J=1-0, HNC J=1-0, plus HC3N J=10-9) and 3mm-continuum using a combination of interferometric ALMA mosaics and IRAM-30m single-dish (SD) maps. Based on our low-resolution (SD) observations, we describe the global properties of our sample covering a wide range of physical conditions including low-, intermediate, and high-mass star-forming regions in different evolutionary stages. Their comparison with ancillary YSO catalogs denotes N$_2$H$^+$ as the best proxy for the dense, star-forming gas in our targets showing a constant star formation efficiency and a fast time evolution of ",

keywords = "astro-ph.GA, astro-ph.SR",

author = "A. Hacar and A. Socci and F. Bonanomi and D. Petry and M. Tafalla and D. Harsono and J. Forbrich and J. Alves and J. Grossschedl and Goicoechea, {J. R.} and J. Pety and A. Burkert and Li, {G. X.}",

note = "{\textcopyright} 2024 The Author(s). Published by EDP Sciences, This is an open access article distributed under the terms of the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/ ",

year = "2024",

month = jul,

day = "5",

doi = "10.1051/0004-6361/202348565",

language = "English",

volume = "687",

pages = "1--37",

journal = "Astronomy & Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

}

Hacar, A, Socci, A, Bonanomi, F, Petry, D, Tafalla, M, Harsono, D, Forbrich, J, Alves, J, Grossschedl, J, Goicoechea, JR, Pety, J, Burkert, A & Li, GX 2024, 'Emergence of high-mass stars in complex fiber networks (EMERGE): I. Early ALMA Survey: Observations and massive data reduction', Astronomy & Astrophysics, vol. 687, A140, pp. 1-37. https://doi.org/10.1051/0004-6361/202348565

TY - JOUR

T1 - Emergence of high-mass stars in complex fiber networks (EMERGE)

T2 - I. Early ALMA Survey: Observations and massive data reduction

AU - Hacar, A.

AU - Socci, A.

AU - Bonanomi, F.

AU - Petry, D.

AU - Tafalla, M.

AU - Harsono, D.

AU - Forbrich, J.

AU - Alves, J.

AU - Grossschedl, J.

AU - Goicoechea, J. R.

AU - Pety, J.

AU - Burkert, A.

AU - Li, G. X.

N1 - © 2024 The Author(s). Published by EDP Sciences, This is an open access article distributed under the terms of the Creative Commons Attribution License (CC BY), https://creativecommons.org/licenses/by/4.0/

PY - 2024/7/5

Y1 - 2024/7/5

N2 - (Abridged) Recent molecular surveys have revealed a rich gas organization of sonic-like fibers in all kind of environments prior to the formation of low- and high-mass stars. This paper introduces the EMERGE project aiming to investigate whether complex fiber arrangements could explain the origin of high-mass stars and clusters. We analyzed the EMERGE Early ALMA Survey including 7 star-forming regions in Orion (OMC-1/2/3/4 South, L1641N, NGC2023, and Flame Nebula) homogeneously surveyed in both molecular lines (N$_2$H$^+$ J=1-0, HNC J=1-0, plus HC3N J=10-9) and 3mm-continuum using a combination of interferometric ALMA mosaics and IRAM-30m single-dish (SD) maps. Based on our low-resolution (SD) observations, we describe the global properties of our sample covering a wide range of physical conditions including low-, intermediate, and high-mass star-forming regions in different evolutionary stages. Their comparison with ancillary YSO catalogs denotes N$_2$H$^+$ as the best proxy for the dense, star-forming gas in our targets showing a constant star formation efficiency and a fast time evolution of

AB - (Abridged) Recent molecular surveys have revealed a rich gas organization of sonic-like fibers in all kind of environments prior to the formation of low- and high-mass stars. This paper introduces the EMERGE project aiming to investigate whether complex fiber arrangements could explain the origin of high-mass stars and clusters. We analyzed the EMERGE Early ALMA Survey including 7 star-forming regions in Orion (OMC-1/2/3/4 South, L1641N, NGC2023, and Flame Nebula) homogeneously surveyed in both molecular lines (N$_2$H$^+$ J=1-0, HNC J=1-0, plus HC3N J=10-9) and 3mm-continuum using a combination of interferometric ALMA mosaics and IRAM-30m single-dish (SD) maps. Based on our low-resolution (SD) observations, we describe the global properties of our sample covering a wide range of physical conditions including low-, intermediate, and high-mass star-forming regions in different evolutionary stages. Their comparison with ancillary YSO catalogs denotes N$_2$H$^+$ as the best proxy for the dense, star-forming gas in our targets showing a constant star formation efficiency and a fast time evolution of

KW - astro-ph.GA

KW - astro-ph.SR

U2 - 10.1051/0004-6361/202348565

DO - 10.1051/0004-6361/202348565

M3 - Article

SN - 0004-6361

VL - 687

SP - 1

EP - 37

JO - Astronomy & Astrophysics

JF - Astronomy & Astrophysics

M1 - A140

ER -

Emergence of high-mass stars in complex fiber networks (EMERGE): I. Early ALMA Survey: Observations and massive data reduction

Abstract

Keywords

Access to Document

Fingerprint

Cite this