Physics
Scientific paper
Nov 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..337..178r&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
Physics
4
Scientific paper
The lifecycles of classical Be star disks are reviewed from an observer's point of view, presenting the spectroscopic evidence concerning the disk formation, evolution, and dissipation. With the exception of hydrodynamic processes during the gradual evolution, all these phases are driven or influenced rather directly by stellar processes. For the disk formation, the stellar processes concerned are rotation, pulsation, and possibly magnetic fields. In particular, the question what fraction is contributed by rotation has been re-opened recently. The disk formation proper, the outburst, has been observed as being rather a discrete than steady process. During the outburst the direct physical connection between star and disk also influences the stellar variability itself. Once the outburst ends, the disk enters a phase of gradual outward evolution. With time, the inner regions of the disk become thinner, turning the disk into a ring with an increasing inner radius. If not replenished by subsequent outbursts, the disk will finally dissipate into the interstellar gas.
No associations
LandOfFree
Links Between Hot Stars and Their 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 Links Between Hot Stars and Their Disks, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Links Between Hot Stars and Their Disks will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1835536