Investigating the Star-forming Sites in the Outer Galactic Arm

Fuente: arXiv
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Main Authors: Verma, Aayushi, Sharma, Saurabh, Dewangan, Lokesh K., Ojha, Devendra K., Mallick, Kshitiz, Yadav, Ram Kesh, Kaur, Harmeen, Chand, Tarak, Agarwal, Mamta, Gupta, Archana
Format: Preprint
Published: 2024
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author Verma, Aayushi
Sharma, Saurabh
Dewangan, Lokesh K.
Ojha, Devendra K.
Mallick, Kshitiz
Yadav, Ram Kesh
Kaur, Harmeen
Chand, Tarak
Agarwal, Mamta
Gupta, Archana
author_facet Verma, Aayushi
Sharma, Saurabh
Dewangan, Lokesh K.
Ojha, Devendra K.
Mallick, Kshitiz
Yadav, Ram Kesh
Kaur, Harmeen
Chand, Tarak
Agarwal, Mamta
Gupta, Archana
contents We aim to investigate the global star formation scenario in star-forming sites AFGL 5157, [FSR2007] 0807 (hereafter FSR0807), [HKS2019] E70 (hereafter E70), [KPS2012] MWSC 0620 (hereafter KPS0620), and IRAS 05331+3115 in the outer galactic arm. The distribution of young stellar objects in these sites coincides with a higher extinction and H2 column density, which agrees with the notion that star formation occurs inside the dense molecular cloud cores. We have found two molecular structures at different velocities in this direction; one contains AFGL 5157 and FSR0807, and the other contains E70, [KPS2012] MWSC 0620, and IRAS 05331+3115. All these clusters in our target region are in different evolutionary stages and might form stars through different mechanisms. The E70 cluster seems to be the oldest in our sample; AFGL 5157 and FSR0807 formed later, and KPS0620 and IRAS 05331+3115 are the youngest sites. AFGL 5157 and FSR0807 are physically connected and have cold filamentary structures and dense hub regions. Additionally, the near-infrared photometric analysis shows signatures of massive star formation in these sites. KPS0620 also seems to have cold filamentary structures with the central hub but lacks signatures of massive stars. Our analysis suggests molecular gas flow and the hub filamentary star formation scenario in these regions. IRAS 05331+3115 is a single clump of molecular gas favoring low-mass star formation. Our study suggests that the selected area is a menagerie of star-forming sites where the formation of the stars happens through different processes.
format Preprint
id arxiv_https___arxiv_org_abs_2406_10388
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Investigating the Star-forming Sites in the Outer Galactic Arm
Verma, Aayushi
Sharma, Saurabh
Dewangan, Lokesh K.
Ojha, Devendra K.
Mallick, Kshitiz
Yadav, Ram Kesh
Kaur, Harmeen
Chand, Tarak
Agarwal, Mamta
Gupta, Archana
Astrophysics of Galaxies
We aim to investigate the global star formation scenario in star-forming sites AFGL 5157, [FSR2007] 0807 (hereafter FSR0807), [HKS2019] E70 (hereafter E70), [KPS2012] MWSC 0620 (hereafter KPS0620), and IRAS 05331+3115 in the outer galactic arm. The distribution of young stellar objects in these sites coincides with a higher extinction and H2 column density, which agrees with the notion that star formation occurs inside the dense molecular cloud cores. We have found two molecular structures at different velocities in this direction; one contains AFGL 5157 and FSR0807, and the other contains E70, [KPS2012] MWSC 0620, and IRAS 05331+3115. All these clusters in our target region are in different evolutionary stages and might form stars through different mechanisms. The E70 cluster seems to be the oldest in our sample; AFGL 5157 and FSR0807 formed later, and KPS0620 and IRAS 05331+3115 are the youngest sites. AFGL 5157 and FSR0807 are physically connected and have cold filamentary structures and dense hub regions. Additionally, the near-infrared photometric analysis shows signatures of massive star formation in these sites. KPS0620 also seems to have cold filamentary structures with the central hub but lacks signatures of massive stars. Our analysis suggests molecular gas flow and the hub filamentary star formation scenario in these regions. IRAS 05331+3115 is a single clump of molecular gas favoring low-mass star formation. Our study suggests that the selected area is a menagerie of star-forming sites where the formation of the stars happens through different processes.
title Investigating the Star-forming Sites in the Outer Galactic Arm
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2406.10388