Velocity variability of semiregular and irregular variables

Author(s)
Thomas Lebzelter, Kenneth H. Hinkle
Abstract

We compare velocities from near infrared lines with center-of-mass velocities for a sample of semiregular and irregular variables to search for indications for a convective blueshift. It is shown that a general blueshift is present but that the light variability is obviously not dominated by convective cells but rather by stellar pulsation. All stars of our sample show a similar shape and amplitude in the velocity variations. Long secondary periods are a common feature in these objects and strongly influence the measured velocity shifts. The star V366 Aq1 is found to be the first SRV showing line doubling.

Organisation(s)
Department of Astrophysics
External organisation(s)
National Optical Astronomy Observatory, Tucson
Journal
Astronomy & Astrophysics
Volume
393
Pages
563-571
No. of pages
9
ISSN
0004-6361
DOI
https://doi.org/10.1051/0004-6361:20021085
Publication date
2002
Peer reviewed
Yes
Austrian Fields of Science 2012
103003 Astronomy
Portal url
https://ucris.univie.ac.at/portal/en/publications/velocity-variability-of-semiregular-and-irregular-variables(cc19c15d-979f-48ce-8804-f190d309dc03).html