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Prog. Theor. Phys. Supplement No.169 (2007) pp. 191-195
Cyclotron Observations of Binary X-Ray Pulsars
Tatehiro Mihara,1,*
Yukikatsu Terada,1
Motoki Nakajima,2
Motoko Suzuki,1
Teruaki Enoto,3
Kazuo Makishima,1,3
Fumiaki Nagase,4
Keisuke Sudoh5 and
the Suzaku Cyclotron Team
1RIKEN, Wako 351-0198, Japan
2Department of Physics, Nihon University, Tokyo 101-8308, Japan
3Department of Physics, The University of Tokyo, Tokyo 113-0033, Japan
4ISAS/JAXA, JAXA-ISAS, Sagamihara 229-8510, Japan
5Department of Physics, Rikkyo University, Tokyo 171-8501, Japan
Abstract:
Suzaku has observed some cyclotron X-ray pulsars in the
SWG (Science working group) phase.
Suzaku detected the cyclotron feature
in the lowest luminosity from A0535+26.
In Her X-1, Suzaku measured new data points
in the year-long trend of cyclotron resonance energy,
and searched for the second harmonic structure.
The RXTE observations of X0331+53 gave the second example on
changing the resonance energy and indicated that the energy ratio
of the 2nd and 1st cyclotron energies is apart from two.
URL :
http://ptp.ipap.jp/link?PTPS/169/191/
DOI : 10.1143/PTPS.169.191
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Citing Article(s) :
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Progress of Theoretical Physics Supplement No.169 (2007) pp. 208-213
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Summary of the “White Dwarf and Neutron Star Isolated and/or Binaries" Session
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Tadayasu Dotani