Spectroscopy of HIP 113790 at the 5th OHP NEON summer school

Autor(en)
Yves Fremat, Antonia Antonova, Michael Lederer
Abstrakt

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(en)
Institut für Astrophysik
Externe Organisation(en)
Royal Observatory of Belgium, Armagh Observatory
Journal
Communications in Asteroseismology
Band
148
Seiten
77-81
Anzahl der Seiten
5
ISSN
1021-2043
DOI
https://doi.org/10.1553/cia148s77
Publikationsdatum
2006
Peer-reviewed
Ja
ÖFOS 2012
103003 Astronomie
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/1d2f9444-833a-4bd3-a78c-ef30eb0b0664