Spectroscopy of HIP 113790 at the 5th OHP NEON summer school
- Author(s)
- Yves Fremat, Antonia Antonova, Michael Lederer
- Abstract
In this contribution, we present the high-resolution observations we obtained for HIP 113790 at the Haute-Provence Observatory using the AURELIE spectrograph. By determing its fundamental parameters, we confirm that the star is located in the ? Scuti instability strip. We further report the detection of rapid line profile variations with a period of about 1.43 hours.
- Organisation(s)
- Department of Astrophysics
- External organisation(s)
- Royal Observatory of Belgium, Armagh Observatory
- Journal
- Communications in Asteroseismology
- Volume
- 148
- Pages
- 77-81
- No. of pages
- 5
- ISSN
- 1021-2043
- DOI
- https://doi.org/10.1553/cia148s77
- Publication date
- 2006
- Peer reviewed
- Yes
- Austrian Fields of Science 2012
- 103003 Astronomy
- Portal url
- https://ucrisportal.univie.ac.at/en/publications/1d2f9444-833a-4bd3-a78c-ef30eb0b0664