activity
19962026
most citedTHINGS: The HI Nearby Galaxy Survey

1.4k citations · 12.9k across the 127 of their papers we have counts for

collaborators

128 papers

astro-ph.GA2026

Star Formation and Accretion in Nearby Galaxies

J. Moldon, A. Alberdi, M. Perez-Torres +11

The appearance of galaxies is strongly dominated by two physical phenomena: star formation and accretion of material onto compact objects, primarily supermassive black holes. Nearb…

astro-ph.GA2025

Stellar Populations and Molecular Gas Composition in the Low-Metallicity Environment of WLM

Haylee N. Archer, Deidre A. Hunter, Bruce G. Elmegreen +8

We investigate the stellar populations and molecular gas properties of a star-forming region within the dwarf irregular (dIrr) galaxy WLM. Low-metallicity dIrrs like WLM offer a va…

astro-ph.GA2025★ 2 cited

Uncovering Extraplanar Gas in UGCA 250 with the Ultra-deep MHONGOOSE Survey

Sushma Kurapati, D. J. Pisano, W. J. G. de Blok +28

We use the neutral atomic hydrogen (HI) observations of the edge-on galaxy UGCA 250, taken as part of the MeerKAT HI Observations of Nearby Galactic Objects - Observing Southern Em…

astro-ph.GA2024★ 2 cited

High-resolution HI mapping of nearby extremely metal-poor blue compact dwarf galaxies

Tom C. Scott, Elias Brinks, Chandreyee Sengupta +1

Optical observations of Blue Compact Dwarf galaxies (BCDs) show they typically have high specific star formation rates and low metallicites. A subset of these galaxies (those with…

astro-ph.GA2024★ 13 cited

MHONGOOSE discovery of a gas-rich low-surface brightness galaxy in the Dorado Group

F. M. Maccagni, W. J. G. de Blok, P. E. Mancera Piña +28

We present the discovery of a low-mass gas-rich low-surface brightness galaxy in the Dorado Group, at a distance of 17.7 Mpc. Combining deep MeerKAT 21-cm observations from the Mee…

astro-ph.GA2023

Molecular and Ionized Gas in Tidal Dwarf Galaxies: The Spatially Resolved Star-Formation Relation

Navyasree Kovakkuni, Federico Lelli, Pierre-alain Duc +12

Tidal dwarf galaxies (TDGs) are low-mass objects that form within tidal and/or collisional debris ejected from more massive interacting galaxies. We use CO() observations from…