activity
19942013
most citedStarbursts and Star Clusters in the Ultraviolet

481 citations · 2.9k across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.CO2013★ 89 cited

New Radial Abundance Gradients for NGC 628 and NGC 2403

Danielle A. Berg, Evan D. Skillman, Donald R. Garnett +5

Motived by recent ISM studies, we present high quality MMT and Gemini spectroscopic observations of H II regions in the nearby spiral galaxies NGC 628 and NGC 2403 in order to meas…

astro-ph.GA2012★ 16 cited

Newly Identified Star Clusters in M33. III. Structural Parameters

Izaskun San Roman, Ata Sarajedini, Jon A. Holtzman +1

We present the morphological properties of 161 star clusters in M33 using the Advanced Camera For Surveys Wide Field Channel onboard the Hubble Space Telescope using observations w…

astro-ph.GA2009★ 26 cited

Newly Identified Star Clusters in M33. II. Radial HST/ACS Fields

Izaskun San Roman, Ata Sarajedini, Donald R. Garnett +1

We present integrated photometry and color-magnitude diagrams for 161 star clusters in M33, of which 115 were previously uncataloged, using the Advanced Camera For Surveys Wide Fie…

astro-ph2005★ 91 cited

Neon and Oxygen Abundances in M33

N. R. Crockett, D. R. Garnett, P. Massey +1

We present new spectroscopic observations of 13 H II regions in the Local Group spiral galaxy M33. The regions observed range from 1 to 7 kpc in distance from the nucleus. Of the 1…

astro-ph2004★ 25 cited

Recombination Line vs. Forbidden Line Abundances in Planetary Nebulae

Mark Robertson-Tessi, Donald R. Garnett

Recombination lines (RLs) of C II, N II, and O II in planetary nebulae (PNs) have been found to give abundances that are much larger in some cases than abundances from collisionall…

astro-ph2004★ 229 cited

Abundances of metal-rich H II regions in M51

Fabio Bresolin, Donald R. Garnett, Robert C. Kennicutt

We have obtained multi-object spectroscopy of H II regions in the spiral galaxy M51 with the Keck I telescope and the Low Resolution Imaging Spectrometer. For 10 objects we have de…