Non-LTE Calculation for the Decretion Disk

Details Non-LTE Calculation for the Decretion Disk Non-LTE Calculation for the Decretion Disk

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aspc..361..249i&link_type=abstract

Active OB-Stars: Laboratories for Stellar and Circumstellar Physics, ASP Conference Series, Vol. 361, Proceedings of the confere

Physics

2

Scientific paper

The non-LTE state of the isothermal steady-state decretion disk around the Be star was calculated by the iteration method. The on-the-spot approximation is adopted for the line transfer, and the continuous radiation is determined through the numerical integration. The decretion disk can reproduce the reasonable V magnitude increase for the mass loss rate less than 10^{-10}M_{odot}yr^{-1} and the observed characteristics of the Balmer line profiles. While, the calculated emission equivalent widths are too small, compared to the observation of π Aqr. Our assumption of T_{d}=2/3 T_{eff} is valid in the case of the optically thin disk, while the disk temperature becomes lower in the optically thick disk.

Affiliated with

Also associated with

No associations

Rating

Non-LTE Calculation for the Decretion Disk 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 Non-LTE Calculation for the Decretion Disk, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Non-LTE Calculation for the Decretion Disk will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-857932