Cyclotron lines in Vela X-1 (Kreykenbohm+, 2002)

Details Cyclotron lines in Vela X-1 (Kreykenbohm+, 2002) Cyclotron lines in Vela X-1 (Kreykenbohm+, 2002)

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ycat..33950129k&link_type=abstract

VizieR On-line Data Catalog: J/A+A/395/129. Originally published in: 2002A&A...395..129K

Physics

X-Ray Sources, Magnetic Fields

Scientific paper

Fitting parameters for the phase resolved spectra of the 2000 and 1998 observation are given. The model in use is the Negative Positive EXponential (NPEX) model (with Gamma2 always fixed to -2, Mihara, 1995, Ph.D. Thesis, Riken, Tokyo) modified by photoelectric absorption, an additive iron line at ~6.4keV, and none, one, or two cyclotron resonant scattering features (CRSF)s at ~25 and ~50keV.
The phase bins for the 2000 observation are: - rise, center, and fall of the main pulse - rise part 1, rise part 2, center, and fall of the secondary pulse - the two inter pulse phases
The phase bins for the 1998 observation are: - rise and fall of the main pulse - rise and fall of the secondary pulse - the two inter pulse phases
(15 data files).

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