activity
20012023
most citedDetection of amino acetonitrile in Sgr B2(N)

290 citations · 3.1k across the 57 of their papers we have counts for

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Showing 2013 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2013★ 50 cited

Evidence for an Interaction in the Nearest Starbursting Dwarf Irregular Galaxy IC 10

David L. Nidever, Trisha Ashley, Colin T. Slater +10

Using deep 21-cm HI data from the Green Bank Telescope we have detected an ~18.3 kpc-long gaseous extension associated with the starbursting dwarf galaxy IC 10. The newly-found fea…

astro-ph.GA2013★ 13 cited

Timescales on which Star Formation Affects the Neutral ISM

Adrienne M. Stilp, Julianne J. Dalcanton, Steven R. Warren +5

Turbulent neutral hydrogen (HI) line widths are often thought to be driven primarily by star formation (SF), but the timescale for converting SF energy to HI kinetic energy is uncl…

astro-ph.GA2013★ 65 cited

Drivers of HI Turbulence in Dwarf Galaxies

Adrienne M. Stilp, Julianne J. Dalcanton, Evan D. Skillman +3

Neutral hydrogen (HI) velocity dispersions are believed to be set by turbulence in the interstellar medium (ISM). Although turbulence is widely believed to be driven by star format…

astro-ph.GA2013★ 12 cited

Nuclear Water Maser Emission in Centaurus A

Juergen Ott, David S. Meier, Mark McCoy +9

We report the detection of a 22GHz water maser line in the nearest (D~3.8Mpc) radio galaxy Centaurus A using the Australia Telescope Compact Array (ATCA). The line is centered at a…

astro-ph.GA2013★ 52 cited

Spectral imaging of the Central Molecular Zone in multiple 7-mm molecular lines

P. A. Jones, M. G. Burton, M. R. Cunningham +2

We have imaged 24 spectral lines in the Central Molecular Zone (CMZ) around the Galactic Centre, in the range 42 to 50 GHz. The lines include emission from the CS, CH3OH, HC3N, SiO…

astro-ph.GA2013★ 48 cited

Global HI Kinematics in Dwarf Galaxies

Adrienne M. Stilp, Julianne J. Dalcanton, Steven R. Warren +3

HI line widths are typically interpreted as a measure of ISM turbulence, which is potentially driven by star formation. In an effort to better understand the possible connections b…