Dec 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010fym..confp..16d&link_type=abstract
"The First Year of MAXI: Monitoring Variable X-ray Sources", Poster Presentations, 4th International MAXI Workshop held November
Other
Scientific paper
We present the results of recent observations of a well known HMXB Vela X-1 with Suzaku and review other observed characteristics of a system with aim to estimate the magnetic field of the neutron star. We conclude, that the observed long pulse period of 283.5 s and its evolution, the "off-states", the observed quasi-periodic oscillations and the noise power spectrum of the X-ray emission may be consistently explained if the neutron star has a magnetic field greater than 1013 G.
Doroshenko Victor
Santangelo Andrea
Suleimanov Valery
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