From the 1 of 8 linked papers with an AI index.
8 papers
The dynamical environment of the high-mass star-forming region G28.2880.364
Jyotirmoy Dey, Devendra K. Ojha, Jagadheep D. Pandian
The paper studies the massive star‑forming region G28.288‑0.364 using multi‑wavelength radio and millimeter data to characterize its ionized gas and dust cores, revealing two compa…
The 10-15 GHz radio continuum survey of the Galactic Plane with SKAO
A. Traficante, C. Mininni, F. Cavallaro +63
Star formation emerges from the complex interplay between gravity, turbulence, magnetic fields, and stellar feedback, all of which vary across spatial scales and Galactic environme…
The Impact and Environment of Massive Stars and Stellar Clusters
Loren Anderson, Jagadheep D. Pandian, Jyotirmoy Dey +10
Massive stars and stellar clusters shape galactic evolution through powerful feedback mechanisms including radiation pressure, photoionization, stellar winds, and cosmic ray accele…
Physical characterization and modeling of candidate Hyper-Compact HII Regions
I. T. RodrÃguez-Esnard, S. Kurtz, J. D. Pandian +4
Hypercompact HII regions (HC) are regions of ionized gas associated with the early stages of high-mass star formation. With the aim of better understanding their characteristics, w…
Detection of non-thermal radio emission components from the Orion Nebula: stellar jets, cloud collision or feedback from stellar winds?
Md Rashid, Nirupam Roy, Prasun Dutta +5
The Orion Nebula is the closest high-mass star-forming region, making it an ideal laboratory to investigate physical processes in complex star-forming environments. At radio freque…
Exploring the interplay between molecular and ionized gas in HII regions
S. Khan, A. M. Jacob, M. R. Rugel +8
We aim to constrain the kinetic temperature and H volume density of massive star-forming clumps associated with HII regions using multiple para-HCO transitions. In addition…