Optical Interferometry and C-rich AGB-Stars

Details Optical Interferometry and C-rich AGB-Stars Optical Interferometry and C-rich AGB-Stars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1001..185h&link_type=abstract

IXTH TORINO WORKSHOP ON EVOLUTION AND NUCLEOSYNTHESIS IN AGB STARS AND THE IIND PERUGIA WORKSHOP ON NUCLEAR ASTROPHYSICS. AIP C

Astronomy and Astrophysics

Astrophysics

2

Carbon Stars, S Stars, And Related Types, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages, Interferometry, Abundances, Chemical Composition, Stellar Atmospheres, Radiative Transfer, Opacity And Line Formation

Scientific paper

We briefly discuss the current capabilities of optical interferometry and its potential to increase our understanding of AGB-stars for such important questions as convection, pulsation, dust formation and mass loss. We then present dynamic model atmospheres for carbon stars and analyze the predicted intensity profiles and visibilities in terms of fits with uniform disks and the current accuracy of visibility measurements. Finally we mention the prospects for real imaging by optical interferometry.

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