Unraveling the Feedback-regulated Star Formation Activities around the Expanding Galactic Mid-infrared Bubble [HKS2019] E71

We explore the physical environment of the Galactic mid-infrared (MIR) bubble [HKS2019] E71 (hereafter E71) through a multiwavelength approach. E71 is located at the edge of a filamentary structure, as traced in Herschel images (250–500 μ m), Herschel column density map, and molecular maps in the ve...

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Bibliografische Detailangaben

Hauptverfasser:	Aayushi Verma, Saurabh Sharma, Lokesh K. Dewangan, Tarak Chand, Ariful Hoque, Devendra K. Ojha, Harmeen Kaur, Ram Kesh Yadav, Mamta, Manojit Chakraborty, Archana Gupta
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	IOP Publishing 2025-01-01
Schriftenreihe:	The Astrophysical Journal
Schlagworte:	Star formation Star forming regions Interstellar medium H II regions Stellar wind bubbles Young stellar objects
Online-Zugang:	https://doi.org/10.3847/1538-4357/adf21d
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