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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A Chandra Spectroscopic Survey of Persistent Black Hole Candidates
TL;DR: In this article, the authors present results from observations of persistent black hole candidates with the High-Energy Transmission Gratings on board the Chandra X-Ray Observatory, including LMC X-1, LMCX-3, GRS 1758-258, and Cyg X 1.
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Intragroup and Galaxy-linked Diffuse X-ray Emission In Hickson Compact Groups
Tyler D. Desjardins,Sarah C. Gallagher,Panayiotis Tzanavaris,John S. Mulchaey,William N. Brandt,Jane C. Charlton,Gordon P. Garmire,Caryl Gronwall,Ann Hornschemeier,Kelsey E. Johnson,Iraklis S. Konstantopoulos,Ann I. Zabludoff +11 more
TL;DR: In this paper, the authors present an archival study of diffuse X-ray emission in a subset of nine Hickson compact groups (HCGs) observed with the Chandra X-Ray Observatory.
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The Field of the TeV Source HESS J1804–216 in X-Rays and Other Wavelengths
TL;DR: In this article, Chandra ACIS data reveal several X-ray sources within the bright part of HESS J1804-216, which are likely associated with nearby stars or distant pulsars.
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Extended x-ray emission in the vicinity of the microquasar ls 5039: pulsar wind nebula?
Martin Durant,Oleg Kargaltsev,George G. Pavlov,George G. Pavlov,Chulhoon Chang,Gordon P. Garmire +5 more
TL;DR: In this paper, Chandra Advanced CCD Imaging Spectrometer observation of LS 5039 provided a high-significance detection of extended emission clearly visible for up to 1' from the point source.
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Anatomy of a Cooling Flow: The Feedback Response to Pure Cooling in the Core of the Phoenix Cluster
Michael McDonald,Brian R. McNamara,G. M. Voit,Matthew B. Bayliss,Bradford Benson,M. Brodwin,R. E. A. Canning,Michael Florian,Gordon P. Garmire,Massimo Gaspari,Michael D. Gladders,Julie Hlavacek-Larrondo,Erin Kara,C. L. Reichardt,Helen Russell,A. Saro,Keren Sharon,Taweewat Somboonpanyakul,Grant R. Tremblay,R. J. van Weeren +19 more
TL;DR: In this paper, Chandra X-ray, optical, and radio observations of the core of the Phoenix cluster are presented, showing that the cooling is highly asymmetric in the inner ~20 kpc and that the bulk of the cooling occurs in a low-entropy filament extending northward from the central galaxy.