Disks and Peculiar Abundances in a Variety of Hot Stars

Details Disks and Peculiar Abundances in a Variety of Hot Stars Disks and Peculiar Abundances in a Variety of Hot Stars

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aspc..337..191j&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

Scientific paper

At least three different classes of hot stars exhibit peculiar surface abundances which can be attributed to accretion from circumstellar dusty rings or disks. In objects with luminosities greater than 10 L&sun;, such as the evolved binary, the Red Rectangle, or the A-type main-sequence star, λ Boo, there appears to be accretion of gas without dust. For the low luminosity (L = 2.4 × 10-3 L&sun;) DA white dwarf, G29-38, there appears to be a dusty ring without much gas, reminiscent of Saturn's rings. Accretion from this ring appears to be detectable in the star's photosphere.

Affiliated with

Also associated with

No associations

Rating

Disks and Peculiar Abundances in a Variety of Hot Stars 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 Disks and Peculiar Abundances in a Variety of Hot Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Disks and Peculiar Abundances in a Variety of Hot Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1835538