Superposition of Cyclotron Lines in Accreting X-Ray Pulsars. II. IncreasingB-Field
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/pasj/article-pdf/65/4/84/17445592/pasj65-0084.pdf
Reference27 articles.
1. Phase dependence of the spectral properties of the X-ray binary 4U0115+63: Observations with the Beppo-Sax satellite
2. Caballero I. 2009, phD thesis, ZAAT University of Tübingen
3. Analyzing X-ray pulsar profiles: geometry and beam pattern of A 0535+26
4. Discovery of a cyclotron absorption line in the spectrum of the binary X-ray pulsar 4U 1538 - 52 observed by GINGA
5. Magnetic Fields of Accreting X‐Ray Pulsars with theRossi X‐Ray Timing Explorer
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1. Variations of magnetic multipoles in the X-ray binary pulsars Her X-1 and A 0535+26;Monthly Notices of the Royal Astronomical Society;2022-03-21
2. Studies of Cepheus X-4 during the 2018 Outburst Observed with AstroSat;The Astrophysical Journal;2021-10-01
3. AstroSat Observations of GRO J2058+42 during the 2019 Outburst;The Astrophysical Journal;2020-07-03
4. The giant outburst of 4U 0115+634 in 2011 with Suzaku and RXTE;Astronomy & Astrophysics;2020-02
5. LAXPC/AstroSat Study of ∼1 and ∼2 mHz Quasi-periodic Oscillations in the Be/X-Ray Binary 4U 0115+63 during Its 2015 Outburst;The Astrophysical Journal;2019-02-07
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