AGB Mass-Loss Variations: What Can We Learn from (Sub)millimetre Observations?

Details AGB Mass-Loss Variations: What Can We Learn from (Sub)millimetre Observations? AGB Mass-Loss Variations: What Can We Learn from (Sub)millimetre Observations?

Jun 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..388..161d&link_type=abstract

Mass Loss from Stars and the Evolution of Stellar Clusters ASP Conference Series, Vol. 388, proceedings of the conference held 2

Astronomy and Astrophysics

Astronomy

Scientific paper

It is generally acknowledged that the mass loss of Asymptotic Giant Branch (AGB) stars undergoes variations on different time scales. We address here the question of the influence of these variations on the spectral energy distribution (SED) of these sources. We therefore constructed models for the dust envelopes for a sample of AGB stars. From the analysis of these dust models, two indications for the presence of mass-loss variations can be found.

Affiliated with

Also associated with

No associations

Rating

AGB Mass-Loss Variations: What Can We Learn from (Sub)millimetre Observations? 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 AGB Mass-Loss Variations: What Can We Learn from (Sub)millimetre Observations?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and AGB Mass-Loss Variations: What Can We Learn from (Sub)millimetre Observations? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-989289