The Circumstellar Envelopes of Be Stars: Viscous Disk Dynamics

Details The Circumstellar Envelopes of Be Stars: Viscous Disk Dynamics The Circumstellar Envelopes of Be Stars: Viscous Disk Dynamics

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..337..249j&link_type=abstract

The Nature and Evolution of Disks Around Hot Stars, ASP Conference Series, Vol. 337, Proceedings of a meeting held 7-9 July 2004

Other

1

Scientific paper

We have constructed axisymmetric models of circumstellar envelopes for Be star disks by successfully combining two numerical codes: a non-LTE radiative transfer code which calculates the level populations and disk temperature distribution self-consistently, and a hydrodynamical code. The output of one code is used as input to the other, and the evolving density and thermal structure of the envelope is followed. The resultant time-dependent temperature, disk density, and velocity distributions are used to investigate the outflowing viscous disk model for Be stars.

Affiliated with

Also associated with

No associations

Rating

The Circumstellar Envelopes of Be Stars: Viscous Disk Dynamics 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 Circumstellar Envelopes of Be Stars: Viscous Disk Dynamics, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The Circumstellar Envelopes of Be Stars: Viscous Disk Dynamics will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1835555