Comment on ``Discovery of the absorption features in the x-ray spectrum of an isolated neutron star''
Jul, 2002Citations per year
Abstract: (arXiv)
In a paper by Sanwal et al. (2002), it is supposed to be very difficult to interpret the absorption features in term of cyclotron lines. However, we would like to address here that the possibility of the absorption being cyclotron resonance can not be ruled out.We propose that the isolate neutron star, 1E 1207.4-5209 in the center of supernova remnant PKS 1209-51/52, has a debris disk and is in a propeller phase, with an accretion rate 6x10^{-11} M_solar/year.References(7)
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