Disk accretion onto weakly magnetized neutron stars

Details Disk accretion onto weakly magnetized neutron stars Disk accretion onto weakly magnetized neutron stars

Oct 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982ans..conf..156c&link_type=abstract

In Max-Planck Inst. Phys. and Astrophys. Accreting Neutron Stars p 156-158 (SEE N83-15179 05-88)

Physics

2

Binary Stars, Deposition, Disk Galaxies, Electromagnetic Spectra, Mass To Light Ratios, Mass Transfer, Neutron Stars, X Ray Sources, Eddington Approximation, Radiant Flux Density, Stellar Luminosity, Stellar Mass, Stellar Spectra, X Ray Spectra

Scientific paper

The physics of the inner accretion disk was studied by low mass X-ray binary systems. It is shown that mass loss from the inner disk explains the X-ray spectrum, X-ray light curve and the fluctuation time scales of the close binary systems Sco X-1, Cyg X-3, 4U 1822-37 and 4U 2129+47. Considerable mass loss always occurs in the more luminous X-ray sources that are close to being Eddington-limited.

Affiliated with

Also associated with

No associations

Rating

Disk accretion onto weakly magnetized neutron stars 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 Disk accretion onto weakly magnetized neutron stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Disk accretion onto weakly magnetized neutron stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1028889