The disc instability model of dwarf-novae and low-mass X-ray binary transients

Details The disc instability model of dwarf-novae and low-mass X-ray binary transients The disc instability model of dwarf-novae and low-mass X-ray binary transients

2001-02-05

arxiv.org/abs/astro-ph/0102072v1

Astronomy and Astrophysics

Astrophysics

102 pages, 36 figures (43 postscript files); New Astronomy Reviews, in press

Scientific paper

10.1016/S1387-6473(01)00112-9

The disc instability model which is supposed to describe outbursts of dwarf
nova and low-mass X-ray binary transient systems is presented and reviewed in
detail. Various deficiencies of the model are pointed out and various remedies
and generalizations are presented and discussed.

Affiliated with

Also associated with

No associations

Rating

The disc instability model of dwarf-novae and low-mass X-ray binary transients 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 The disc instability model of dwarf-novae and low-mass X-ray binary transients, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The disc instability model of dwarf-novae and low-mass X-ray binary transients will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-104462