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G. P. Garmire

4 papers here

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • middle author2
  • last author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph4
ORCID 0000-0002-7371-5416

identity via Semantic Scholar / OpenAlex

activity
20032008
most citedX-ray flares in Orion young stars. I. Flare characteristics

140 citations · 301 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph2008★ 140 cited

X-ray flares in Orion young stars. I. Flare characteristics

Konstantin V. Getman, Eric D. Feigelson, Patrick S. Broos +2

Pre-main sequence (PMS) stars are known to produce powerful X-ray flares which resemble magnetic reconnection solar flares scaled by factors up to 10^4. However, numerous puzzles a…

astro-ph2007★ 93 cited

Polarized NIR and X-ray Flares from SgrA*

A. Eckart, F. K. Baganoff, M. Zamaninasab +18

Stellar dynamics indicate the presence of a super massive 3-4x10^6 Msun solm black hole at the Galactic Center. It is associated with the variable radio, near-infrared, and X-ray c…

astro-ph2006★ 27 cited

Discovery of a Candidate Central Compact Object in the Galactic Nonthermal SNR G330.2+1.0

Sangwook Park, Koji Mori, Oleg Kargaltsev +5

We report on the discovery of a pointlike source (CXOU J160103.1−513353) at the center of a Galactic supernova remnant (SNR) G330.2+1.0 with {\it Chandra X-Ray Observatory}. The…

astro-ph2003★ 41 cited

0103-72.6: A New Oxygen-Rich Supernova Remnant in the Small Magellanic Cloud

Sangwook Park, John P. Hughes, David N. Burrows +3

0103−72.6, the second brightest X-ray supernova remnant (SNR) in the Small Magellanic Cloud (SMC), has been observed with the {\it Chandra X-Ray Observatory}. Our {\it Chandra} o…

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