Unified model fitting to variable X-ray spectra of Cygnus X-3

Details Unified model fitting to variable X-ray spectra of Cygnus X-3 Unified model fitting to variable X-ray spectra of Cygnus X-3

Mar 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993mnras.261..353n&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 261, no. 2, p. 353-365.

Astronomy and Astrophysics

Astronomy

23

Stellar Models, X Ray Binaries, X Ray Spectra, Accretion Disks, Ginga Satellite

Scientific paper

A unified X-ray spectral model which can be fitted to any of the spectra observed with Ginga is presented. The model consists of three components: an absorbed power-law component modified with an exponential cutoff at high energy, an absorbed blackbody component, and an iron emission line. The best-fitting values of parameters obtained using the model are given, and the interpretation of the physical meaning of these parameters is described.

Affiliated with

Also associated with

No associations

Rating

Unified model fitting to variable X-ray spectra of Cygnus X-3 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Unified model fitting to variable X-ray spectra of Cygnus X-3, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Unified model fitting to variable X-ray spectra of Cygnus X-3 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1705785