activity
20152019
most citedUnique Tracks Drive the Scatter of the Spatially-Resolved Star Formation Main Sequence

28 citations · 93 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2019★ 14 cited

The radial distribution of supernovae compared to star formation tracers

Fiona M. Audcent-Ross, Gerhardt R. Meurer, James R. Audcent +5

Given the limited availability of direct evidence (pre-explosion observations) for supernova (SN) progenitors, the location of supernovae (SNe) within their host galaxies can be us…

astro-ph.GA2018★ 13 cited

The Neutral Hydrogen Properties of Galaxies in Gas-rich Groups

Robert Džudžar, Virginia Kilborn, Gerhardt Meurer +23

We present an analysis of the integrated neutral hydrogen (HI) properties for 27 galaxies within nine low mass, gas-rich, late-type dominated groups which we denote "Choirs". We fi…

astro-ph.GA2018★ 28 cited

Unique Tracks Drive the Scatter of the Spatially-Resolved Star Formation Main Sequence

Christine Hall, Stephane Courteau, Thomas Jarrett +4

The scatter of the spatially resolved star formation main sequence (SFMS) is investigated in order to reveal signatures about the processes of galaxy formation and evolution. We ha…

astro-ph.GA2018★ 9 cited

Near-identical star formation rate densities from H and FUV at redshift zero

Fiona M. Audcent-Ross, Gerhardt R. Meurer, O. I. Wong +27

For the first time both H and far-ultraviolet (FUV) observations from an HI-selected sample are used to determine the dust-corrected star formation rate density (SFRD: )…

astro-ph.GA2018★ 21 cited

Cosmic clocks: A Tight Radius - Velocity Relationship for HI-Selected Galaxies

Gerhardt R. Meurer, Danail Obreschkow, O. Ivy Wong +3

HI-Selected galaxies obey a linear relationship between their maximum detected radius Rmax and rotational velocity. This result covers measurements in the optical, ultraviolet, and…

astro-ph.GA2015★ 8 cited

Kinematics of dwarf galaxies in gas-rich groups, and the survival and detectability of tidal dwarf galaxies

Sarah M. Sweet, Michael J. Drinkwater, Gerhardt Meurer +4

We present DEIMOS multi-object spectroscopy (MOS) of 22 star-forming dwarf galaxies located in four gas-rich groups, including six newly-discovered dwarfs. Two of the galaxies are…