G
Gordon P. Garmire
Researcher at Pennsylvania State University
Publications - 493
Citations - 38165
Gordon P. Garmire is an academic researcher from Pennsylvania State University. The author has contributed to research in topics: Galaxy & Luminosity. The author has an hindex of 99, co-authored 485 publications receiving 36277 citations. Previous affiliations of Gordon P. Garmire include Harvard University.
Papers
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The Elephant Trunk Nebula and the Trumpler 37 cluster: contribution of triggered star formation to the total population of an HII region
Konstantin V. Getman,Eric D. Feigelson,Aurora Sicilia-Aguilar,Patrick S. Broos,Michael A. Kuhn,Gordon P. Garmire +5 more
TL;DR: In this paper, a spatio-temporal gradient of stars from the IC 1396A cloud toward the primary ionizing star HD 206267 is found, and the authors argue that the TSF mechanism is the radiation-driven implosion process persisting over several million years.
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Chandra Observations of Radio-Loud Quasars at z > 4: X-Rays from the Radio Beacons of the Early Universe
Lee C. Bassett,W. N. Brandt,Donald P. Schneider,Cristian Vignali,Cristian Vignali,George Chartas,Gordon P. Garmire +6 more
TL;DR: In this paper, Chandra observations of six radio-loud quasars (RLQs) and one optically bright radio-quiet quasar (RQQ) at z 4.1.4.
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An X-ray Imaging Study of the Stellar Population in RCW49
Masahiro Tsujimoto,E. D. Feigelson,Leisa K. Townsley,Patrick S. Broos,Konstantin V. Getman,Jing Wang,Gordon P. Garmire,Daisuke Baba,Takahiro Nagayama,Motohide Tamura,Ed Churchwell +10 more
TL;DR: In this article, a high-resolution X-ray imaging study of the stellar population in the Galactic massive star-forming region RCW49 and its central OB association Westerlund 2 is presented.
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A Chandra Observation of the Obscured Star-Forming Complex W40
Michael A. Kuhn,Konstantin V. Getman,Eric D. Feigelson,Bo Reipurth,Steven A. Rodney,Gordon P. Garmire +5 more
TL;DR: In this article, the authors detect 225 X-ray sources, of which 85% are confidently identified as young stellar members of the W40 H II region, and two potential distances of the cluster, 260 pc and 600 pc, are used in the paper.
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X-Ray Source Population in the Elliptical Galaxy NGC 720 with Chandra
TL;DR: In this article, the authors detect 42 X-ray point sources in the elliptical galaxy NGC 720, including a possible central source, and investigate both the hardness ratios and combined spectra of the sources.