Accretion Processes in Mira AB

Details Accretion Processes in Mira AB Accretion Processes in Mira AB

Jul 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004rmxac..20...92k&link_type=abstract

Compact Binaries in the Galaxy and Beyond, Proceedings of the conference held 17-22 November, 2003 in La Paz, Baja California Su

Astronomy and Astrophysics

Astronomy

1

Accretion, Accretion Disks, Stars: Agb And Post Agb, Stars: Mass Loss

Scientific paper

The Mira AB interacting binary provides an ideal laboratory for studying mass loss and accretion processes in systems containing an AGB star and a compact accretor, because its components have been resolved and can be studied individually. We present here results from our long term study of accretion processes in this system. These include recent HST observations suggesting that the accretion rate onto Mira B is much lower than before, indicating possible disruption of the accretion disk.

Affiliated with

Also associated with

No associations

Rating

Accretion Processes in Mira AB 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 Accretion Processes in Mira AB, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Accretion Processes in Mira AB will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-771817