VLTI observations of AGB stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

5 pages, to appear in the proceedings of the workshop "Stellar end products", Granada, 13-15 April 2005, Mem. S. A. It, submit

Scientific paper

We report on recent observations of AGB stars obtained with the VLT Interferometer (VLTI). We illustrate in general the potential of interferometric measurements to study stellar atmospheres and circumstellar envelopes, and demonstrate in particular the advantages of a coordinated multi-wavelength approach including near/mid-infrared as well as radio interferometry. We report on studies of the atmospheric structure of non-Mira and Mira variable giants. We have used VLTI observations of the near- and mid-infrared stellar sizes and concurrent VLBA observations of the SiO maser emission. So far, this project includes studies of the Mira stars S Ori and RR Aql as well as of the supergiant AH Sco. The results from our first epochs of S Ori measurements have recently been published and the main results are reviewed here. The S Ori maser ring is found to lie at a mean distance of approximately 2 stellar radii, a result that is virtually free of the usual uncertainty inherent in comparing observations of variable stars widely separated in time and stellar phase. We discuss the status of our more recent S Ori, RR Aql, and AH Sco observations, and present an outlook on the continuation of our project.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

VLTI observations of AGB 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 VLTI observations of AGB stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and VLTI observations of AGB stars will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-163984

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.