collaborators

5 papers

astro-ph.HE2026

Supernova remnants in the new radio astronomy era

A. Ingallinera, M. Arias, G. Castelletti +25

Supernova remnants (SNRs) are what is left after stellar explosions, when the stellar ejecta, the explosion shock and the circumstellar medium interact. Despite being among the fir…

astro-ph.GA2025

The SOMA MM Survey. I. An Astrochemical Census of Massive Protostars

D. Gigli, P. Gorai, C. Y. Law +9

During massive star formation, dense gas undergoes chemical evolution, producing both simple and complex organic molecules (COMs) characteristic of hot molecular cores. How this ev…

astro-ph.SR2025

The SOFIA Massive (SOMA) Star Formation Q-band Follow-up. II. Hydrogen Recombination Lines Toward High-Mass Protostars

Prasanta Gorai, Kotomi Taniguchi, Jonathan C. Tan +11

Hydrogen recombination lines (HRLs) are valuable diagnostics of the physical conditions in ionized regions around high-mass stars. Understanding their broadening mechanisms and int…

astro-ph.GA2025

The SOFIA Massive (SOMA) Star Formation Survey. V. Clustered Protostars

Zoie Telkamp, Ruben Fedriani, Jonathan C. Tan +16

We present m SOFIA-FORCAST images of seven regions of ``clustered" star formation as part of the SOFIA Massive (SOMA) Star Formation Survey. We identify a total of 34…

astro-ph.GA2025

The Core Mass Function Across Galactic Environments. IV. The Galactic Center

Alva V. I. Kinman, Maya A. Petkova, Jonathan C. Tan +2

The origin of the stellar Initial Mass Function (IMF) and how it may vary with galactic environment is a matter of debate. Certain star formation theories involve a close connectio…