A note on the discovery of absorption features in 1E 1207.4-5209

Details A note on the discovery of absorption features in 1E 1207.4-5209 A note on the discovery of absorption features in 1E 1207.4-5209

2002-07-03

arxiv.org/abs/astro-ph/0207079v2

Chin.Phys.Lett. 20 (2003) 314-316

Astronomy and Astrophysics

Astrophysics

4 page and 1 figure, revised substantially, or at http://vega.bac.pku.edu.cn/~rxxu/publications/index_P.htm

Scientific paper

10.1088/0256-307X/20/2/343

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.

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