Investigating the physical conditions in extended system hosting mid-infrared bubble N14
L. K. Dewangan, T. Baug, L. E. Pirogov, D. K. Ojha

TL;DR
This study uses multi-wavelength observations to analyze the physical conditions and star formation activity in an extended molecular system associated with the mid-infrared bubble N14, revealing signs of fragmentation and collapse.
Contribution
It provides a detailed multi-wavelength analysis of a large-scale environment around N14, highlighting the role of global collapse and fragmentation in star formation.
Findings
Extended physical system of ~59x29 pc hosting star-forming clumps.
Presence of non-thermal emission and young ionized clumps.
Velocity oscillations indicating fragmentation and collapse.
Abstract
To observationally explore physical processes, we present a multi-wavelength study of a wide-scale environment toward l = 13.7 - 14.9 degrees containing a mid-infrared bubble N14. The analysis of 12CO, 13CO, and C18O gas at [31.6, 46] km/s reveals an extended physical system (extension ~59 pc x 29 pc), which hosts at least five groups of the ATLASGAL 870 micron dust clumps at d ~3.1 kpc. These spatially-distinct groups/sub-regions contain unstable molecular clumps, and are associated with several Class I young stellar objects (mean age ~0.44 Myr). At least three groups of ATLASGAL clumps associated with the expanding HII regions (including the bubble N14) and embedded infrared dark clouds, devoid of the ionized gas, are found in the system. The observed spectral indices derived using the GMRT and THOR radio continuum data suggest the presence of non-thermal emission with the HII…
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