2022
DOI: 10.3847/1538-4357/ac3a78
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A Comprehensive Study of the Young Cluster IRAS 05100+3723: Properties, Surrounding Interstellar Matter, and Associated Star Formation

Abstract: We present a comprehensive multiwavelength investigation of a likely massive young cluster “IRAS 05100+3723” and its environment with the aim to understand its formation history and feedback effects. We find that IRAS 05100+3723 is a distant (∼3.2 kpc), moderate-mass (∼500 M ⊙), young (∼3 Myr) cluster with its most massive star being an O8.5V type. From spectral modeling, we estimate the effective temperature and log g of the star to be ∼33,000 K and ∼3.8, respectively. Our radio continuum ob… Show more

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Cited by 4 publications
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“…It is a vast region in which star formation is active. A young cluster IRAS 05100 +3723 is associated with the H II region S228 (Yadav et al 2022). The heliocentric distance of this target is 2.56 ± 0.09 kpc, and the corresponding Galactocentric distance R G = 10.72 ± 0.19 kpc.…”
Section: A4 Sh2-228mentioning
confidence: 98%
“…It is a vast region in which star formation is active. A young cluster IRAS 05100 +3723 is associated with the H II region S228 (Yadav et al 2022). The heliocentric distance of this target is 2.56 ± 0.09 kpc, and the corresponding Galactocentric distance R G = 10.72 ± 0.19 kpc.…”
Section: A4 Sh2-228mentioning
confidence: 98%