X ray nova GS 2000+25 = Nova VUL 1988: X ray and optical light curves, spectra, and model

Details X ray nova GS 2000+25 = Nova VUL 1988: X ray and optical light curves, spectra, and model X ray nova GS 2000+25 = Nova VUL 1988: X ray and optical light curves, spectra, and model

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989esasp.296..305b&link_type=abstract

In ESA, The 23rd ESLAB Symposium on Two Topics in X Ray Astronomy. Volume 1: X Ray Binaries p 305-309 (SEE N90-25711 19-89)

Astronomy and Astrophysics

Astronomy

4

Accretion Disks, Light Curve, Stellar Models, X Ray Binaries, X Ray Spectra, Light (Visible Radiation), Mir Space Station, Stellar Mass, Stellar Mass Accretion, X Ray Astronomy

Scientific paper

The results of optical and X-ray observations of X-ray Nova Vul 1988 are presented. The observations, performed on the module Kvant, revealed a soft and a hard component of the X-ray spectrum. The discussion is carried out in the framework of the model of nonstationary disc accretion. The assumption on the disk accretion taking place onto a black hole of stellar mass is made.

Affiliated with

Also associated with

No associations

Rating

X ray nova GS 2000+25 = Nova VUL 1988: X ray and optical light curves, spectra, and model 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 X ray nova GS 2000+25 = Nova VUL 1988: X ray and optical light curves, spectra, and model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X ray nova GS 2000+25 = Nova VUL 1988: X ray and optical light curves, spectra, and model will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1614523