Luminosity, redshift and gas abundance in general relativistic radiation hydrodynamics

Details Luminosity, redshift and gas abundance in general relativistic radiation hydrodynamics Luminosity, redshift and gas abundance in general relativistic radiation hydrodynamics

2008-06-13

arxiv.org/abs/0806.2240v1

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

3 figures

Scientific paper

Quasi-stationary flows of gas accreting onto a compact center are analyzed in the framework of general-relativistic radiation hydrodynamics, under assumptions of spherical symmetry and thin gas approximation. Numerical investigation shows that luminosity, redshift and gas abundance are correlated. The gas can constitute up to one third of the total mass of brightest low-redshift sources, but its abundance goes down to 1/30 for sources with luminosities close to the Eddington limit.

Affiliated with

Also associated with

No associations

Rating

Luminosity, redshift and gas abundance in general relativistic radiation hydrodynamics 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 Luminosity, redshift and gas abundance in general relativistic radiation hydrodynamics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Luminosity, redshift and gas abundance in general relativistic radiation hydrodynamics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-123328