Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
Bogazici University, Istanbul, Turkey
Sabancı University, 34956, Orhanlı Tuzla, İstanbul, Turkey
Sabancı University, Orhanlı, Tuzla 34956, Istanbul, Turkey
Sabanci University
Middle East Technical University
Sabanci University, Istanbul, Turkey
FENS, Sabanci University, Turkey
Sabanci Univ., Istanbul;
Sabanci Univ. Istanbul
Scientific and Technical Research Council of Turkey, Research Institute for Basic Sciences, P.K. 74, Gebze, Kocaeli 41470, Turkey
Scientific and Technical Research Council of Turkey, Research Institute for Basic Sciences, Gebze
Middle East Technical University, Ankara, Turkey
Scientific and Technical Research Council of Turkey, Research Institute for Basic Sciences, Gebze; Illinois, University, Urbana
Sabanci University, Turkey
API, University of Amsterdam
Faculty of Engineering and Natural Sciences, Sabanci University, Istanbul, Turkey
Middle East Technical University, Physics Department, 06531, Ankara, Turkey
Columbia University, New York, NY; Bogazici University, Istanbul, Turkey
Univ. Cambridge, UK
Illinois Univ., Urbana-Champaign.
Physics Department, Middle East Technical University, Ankara 06531, Turkey
Illinois, University, Urbana, IL
Middle East Technology Univ., Ankara, Turkey
Faculty of Engineering and Natural Sciences, Sabancı University, Orhanlı, Tuzla, Istanbul 34956, Turkey
Bogazici University, Istanbul, Turkey; Illinois, University, Urbana, IL
Sabancı University, Orhanlı-Tuzla, İstanbul, 34956, Turkey
Illinois, University, Urbana
Sabancı University, Orhanlı-Tuzla 34956, İstanbul / Turkey
Scientific and Technical Research Council of Turkey, Research Institute for Basic Science, Gebze
Columbia University, New York, NY; I
6 HZ quasiperiodic oscillations from low-mass X-ray binaries - The sound of an accretion disk?
A Natural Limit on the Observable Periods of Anomalous X-ray Pulsars and Soft Gamma-ray Repeaters
A new class of radio pulsars
A New Class of Radio Pulsars - Back in 1982
A search for X-rays from five pulsars: PSR's 0740-28, 1737-30, 1822-09, 1915+13 and 1916+14
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