collaborators

6 papers

astro-ph.GA2026

The EDGE-CALIFA Survey: Star Formation Efficiency and Galaxy Quenching across 62 Main Sequence, Green Valley, and Red Galaxies

Yu-Hsuan Teng, Alberto D. Bolatto, Peter J. Teuben +26

We present GBT-EDGE, a new CO(1-0) survey using the Green Bank Telescope to map 62 nearby (10-140 Mpc) galaxies spanning the star-forming main sequence (SFMS), green valley, and re…

astro-ph.CO2026

The local ultraviolet signature of Type Ia supernova environments from HST and MUSE

Lluís Galbany, Lluís Galbany, Cullen Abelson +22

The local environment of a Type Ia supernova (SN~Ia) traces the local stellar-population age (a statistical proxy for the progenitor age), star formation, dust, and chemical enrich…

astro-ph.GA2025

SDSS-V Local Volume Mapper (LVM): Revealing the Structure of the Rosette Nebula

Mónica A. Villa-Durango, Jorge Barrera-Ballesteros, Carlos G. Román-Zúñiga +19

The Rosette Nebula is a well-known H II region shaped by the interaction of gas with the OB stars of the NGC 2244 stellar association. Located within the remnant of a giant molecul…

astro-ph.GA2025

Physical properties of gas departing from circular rotation at 50 pc scales using the PHANGS-MUSE galaxies

Carlos López-Cobá, Lihwai Lin, Irene Cruz González +4

Noncircular motions have been observed across various spatial scales in disk galaxies, yet the physical properties of the gas involved in these motions remain poorly constrained. U…

astro-ph.GA2025

The vertical structure of the stellar disk in NGC 551

Harshal Raut, Narendra Nath Patra, Prerana Biswas +6

We self-consistently determine the 3D density distribution of NGC 551's stellar disk and study observational signatures of two-component stellar disks. Assuming baryonic disks are…

astro-ph.GA2025

Nebular emission from composite star-forming galaxies -- I. A novel modelling approach

Christophe Morisset, Stéphane Charlot, Sebastián F. Sánchez +3

We introduce a novel approach to modelling the nebular emission from star-forming galaxies by combining the contributions from many HII regions incorporating loose trends in physic…