Doppler Tomograms from Hydrodynamical Models of Dwarf Nova Disks

Details Doppler Tomograms from Hydrodynamical Models of Dwarf Nova Disks Doppler Tomograms from Hydrodynamical Models of Dwarf Nova Disks

2003-02-24

arxiv.org/abs/astro-ph/0302478v1

Astronomy and Astrophysics

Astrophysics

accepted for publication by Acta Astronomica

Scientific paper

We present three-dimensional models of accretion disks in U Gem - like systems and calculate their Doppler tomograms. The tomograms are based on two different assumptions concerning the origin of line emission from the disk. The assumption of lines originating due to irradiation of the surface layer of the disk by the central source leads to a better agreement with observations. We argue that fully three-dimensional modelling is necessary to properly interpret the observed tomograms.

Affiliated with

Also associated with

No associations

Rating

Doppler Tomograms from Hydrodynamical Models of Dwarf Nova Disks 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 Doppler Tomograms from Hydrodynamical Models of Dwarf Nova Disks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Doppler Tomograms from Hydrodynamical Models of Dwarf Nova Disks will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-544789