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20112018
most citedHI Kinematics Along The Minor Axis of M82

63 citations · 230 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2018★ 63 cited

A high-resolution mosaic of the neutral hydrogen in the M81 triplet

W. J. G. de Blok, Fabian Walter, Annette M. N. Ferguson +10

We present a 3x3 degrees, 105-pointing, high-resolution neutral hydrogen (HI) mosaic of the M81 galaxy triplet (including the galaxies M81, M82 and NGC 3077, as well as dwarf galax…

astro-ph.GA2018★ 63 cited

HI Kinematics Along The Minor Axis of M82

Paul Martini, Adam K. Leroy, Jeffrey G. Mangum +4

M82 is one of the best studied starburst galaxies in the local universe, and is consequently a benchmark for studying star formation feedback at both low and high redshift. We pres…

astro-ph.GA2014★ 41 cited

A low HI column density filament in NGC 2403: signature of interaction or accretion

W. J. G. de Blok, Katie M. Keating, D. J. Pisano +6

Observed HI accretion around nearby galaxies can only account for a fraction of the gas supply needed to sustain the currently observed star formation rates. It is possible that ad…

astro-ph.CO2012★ 55 cited

The HI environment of the M101 group

Chris Mihos, Katie Keating, Kelly Holley-Bockelmann +2

We present a wide (8.5x6.7 degree, 1050x825 kpc), deep (sigma(N_HI)=10^(16.8-17.5) cm^-2) neutral hydrogen (HI) map of the M101 galaxy group. We identify two new HI sources in the…

astro-ph.IM2012★ 2 cited

Search for Electromagnetic Counterparts to LIGO-Virgo Candidates: Expanded Very Large Array

Joseph Lazio, Katie Keating, F. A. Jenet +3

This paper summarizes a search for radio wavelength counterparts to candidate gravitational wave events. The identification of an electromagnetic counterpart could provide a more c…

astro-ph.GA2011

The Structure of NGC 1976 in the Radio Range, v2

T. L. Wilson, S. Casassus, Katie M. Keating

High angular resolution radio continuum images of NGC 1976 (M42, Orion A) at frequency=330 MHz (wavelength=91 cm), 1.5 GHz (20 cm) and 10.6 GHz (2.8 cm), have been aligned, placed…

physics.space-ph2011★ 6 cited

The Structure of NGC 1976 in the Radio Range

T. L. Wilson, S. Casassus, Katie M. Chynoweth

High angular resolution radio continuum images of NGC 1976 (M42, Orion A) at frequency=330 MHz (wavelength=91 cm), 1.5 GHz (20 cm) and 10.6 GHz (2.8 cm), have been aligned, placed…