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From the 1 of 9 linked papers with an AI index.

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9 papers

astro-ph.GA2026

Low-Metallicity Star Formation Survey in Sh2-284 (LZ-STAR): The Core Mass Function

Yu Cheng, Jonathan C. Tan, Morten Andersen +4

The authors use ALMA 1.3 mm dust continuum observations of the low‑metallicity star‑forming region Sh2‑284 to identify dense cores and measure the core mass function, finding a hig…

astro-ph.SR2026

The SOMA Atomic Outflow Survey. I. An Atomic OI and Highly Ionized OIII Outflow from Massive Protostar G11.94-00.62

Phillip Oakey, Yao-Lun Yang, Jonathan C. Tan +7

Massive stars regulate galaxy evolution and star formation through their physical and chemical feedback, but their formation remains poorly understood. Accretion-powered outflows p…

astro-ph.GA2026

MAGellanic Outflow and chemistry Survey (MAGOS): Hot cores in the LMC

Takashi Shimonishi, Kei E. I. Tanaka, Yichen Zhang +3

The Large Magellanic Cloud (LMC) provides a key laboratory for exploring the diversity of star formation and interstellar chemistry under subsolar metallicity conditions. We presen…

astro-ph.GA2026

Digging into the chemical complexity in the outer Galaxy: A hot molecular core in Sharpless 2-283

Toki Ikeda, Takashi Shimonishi, Hiroyuki Kaneko +3

The outer Galaxy (galactocentric distance 13.5 kpc) serves as an excellent laboratory for investigating the chemical complexity in low-metallicity environments. Here, we p…

astro-ph.GA2025

ALMA Observations of Cold Methanol Gas in the Large Magellanic Cloud (LMC): N79 South GMC

Suman Kumar Mondal, Takashi Shimonishi, Soumen Mondal +4

We report ALMA continuum and molecular line observations at 0.1 pc resolution toward the super star cluster (SSC) candidate H72.97-69.39 in the N79 region of the LMC. The continuum…

astro-ph.SR2025

The SOFIA Massive (SOMA) Radio Survey. II. Radio Emission from High-Luminosity Protostars

Francisco Sequeira-Murillo, Viviana Rosero, Joshua Marvil +9

We present centimeter continuum observations of seven high luminosity massive protostars and their surrounding sources in regions with multiple targets, as part of the SOFIA Massiv…