Variability of X-ray emission from CEN X-3 observed with GINGA

Details Variability of X-ray emission from CEN X-3 observed with GINGA Variability of X-ray emission from CEN X-3 observed with GINGA

Dec 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.210..113k&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 210, no. 1-2, p. 113-115 (IAU Colloquium 134)

Astronomy and Astrophysics

Astrophysics

Accretion Disks, Chaos, Stellar Models, Stellar Oscillations, X Ray Sources, Emission Spectra, Ginga Satellite, Light Curve, Periodic Variations

Scientific paper

Simplified stellar models like one-zone models can be oscillated in
chaotic state (Saitou et al. 1989). It is natural to consider that the
irregular variations of Galactic X-ray sources might be caused by
nonlinear oscillation of accretion disks or related flow. We studied the
variability of Cen X-3 and applied the nonlinear theory to it.

Affiliated with

Also associated with

No associations

Rating

Variability of X-ray emission from CEN X-3 observed with GINGA 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 Variability of X-ray emission from CEN X-3 observed with GINGA, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Variability of X-ray emission from CEN X-3 observed with GINGA will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-783646