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.GA2025

The EDGE-CALIFA Survey: Influence of Mergers on Radial Profiles of Star-Formation Properties

Y. Garay-Solis, J. K. Barrera-Ballesteros, L. Carigi +6

In this study, we investigate how the merging process influences the radial variations of the specific Star Formation Rate (sSFR), Star Formation Efficiency (SFE), and molecular ga…

astro-ph.GA2025

LMC+: Large-scale mapping of [CII] and [OIII] in the LMC molecular ridge, I. Dataset and line ratio analyses

C. Fischer, S. C. Madden, A. Krabbe +29

The fundamental process of star formation in galaxies involves the interplay between the fueling of star formation via molecular gas and the feedback from recently formed massive s…

astro-ph.GA2025

The EDGE-CALIFA survey: The effect of active galactic nucleus feedback on the integrated properties of galaxies at different stages of their evolution

Z. Bazzi, D. Colombo, F. Bigiel +5

Galaxy quenching, the intricate process through which galaxies transition from active star-forming states to retired ones, remains a complex phenomenon that requires further invest…

astro-ph.GA2025

The EDGE-CALIFA survey: Star formation relationships for galaxies at different stages of their evolution

D. Colombo, V. Kalinova, Z. Bazzi +13

Galaxy evolution is largely driven by star formation activity or by the cessation of it, also called star formation quenching. In this paper, we present star formation scaling rela…

astro-ph.GA2025

The EDGE-CALIFA Survey: An integral field unit-based integrated molecular gas database for galaxy evolution studies in the Local Universe

D. Colombo, V. Kalinova, Z. Bazzi +14

Studying galaxy evolution requires knowledge not only of the stellar properties, but also of the interstellar medium (in particular the molecular phase) out of which stars form, us…