Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
NASA / GSFC and UMBC
NASA / GSFC USA
NASA GSFC
NASA / GSFC and USRA
Keele University
NASA / GSFC and Usra
CRESST and NASA / GSFC
Code 662, NASA Goddard Space Flight Center, Greenbelt, MD 20771
Universities Space Research Association
London, University College, Dorking, England
Oxford University; London, University College, Dorking, England
NASA / GSFC, USRA
UMBC and NASA / GSFC / CRESST
Penn State University, University Park, PA, US
NASA. Goddard Space Flight Center, Greenbelt, MD, US
Laboratory for High Energy Astrophysics, Code 668, NASA-Goddard Space Flight Center, Greenbelt, MD 20771, USA
Laboratory for High Energy Astrophysics, Code 662, NASA Goddard Space Flight Center, Greenbelt, MD 20771 and X-ray Astrophysics Laboratory, NASA / GSFC, Greenbelt, MD 20771, USA
NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA
NASA / GSFC, USRA, Columbia University
NASA / GSFC, Code 668, Greenbelt MD 20771, USA
Exploration of the Universe Division, NASA / Goddard Space Flight Center, Greenbelt, MD 20771, USA
USRA, NASA / GSFC
Institute of Space and Astronautical Science, Sagamihara, Japan
Laboratory for High Energy Astrophysics, Greenbelt, MD, US
California, University, Berkeley
California Univ., Berkeley
NASA, Goddard Space Flight Center, Greenbelt, MD
Tokyo Univ., Japan
Exploration of the Universe Division, Code 660, NASA / GSFC, Greenbelt, MD 20771, USA
Laboratory for High Energy Astrophysics, Goddard Space Flight Center, National Aeronautics and Space Administration, MS 660.2, Greenbelt, MD 20771 for High Energy Astrophysics, NASA Goddard Space Flight Center, Code 662, Greenbelt, MD 20771; Universities Space Research Association.
A burst from the direction of UZ Fornacis with XMM-Newton
A new soft X-ray mode in the AM Herculis object E2003 + 225
A new two channel high-speed photo-polarimeter (HIPPO) for the SAAO
A ROSAT PSPC observation of the eclipsing AM HER cataclysmic variable EP Draconis (=H1907+690)
Accretion streams in AM HER type systems
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