A new photometric study of the high galactic latitude ? Cephei star HN Aqr

Autor(en)
Gerald Handler, R R Shobbrook
Abstrakt

We have carried out 32 h of new time-resolved CCD UBV photometry of the high galactic latitude ? Cephei star HN Aqr. We detected its known single pulsation frequency and noticed additional variability at lower frequencies. It is not clear whether or not this longer-term variation originates from HN Aqr itself. The UBV colour amplitudes of the star's ? Cephei pulsation point towards an l=4 or l=2 mode, inconsistent with previous mode identifications.

Organisation(en)
Institut für Astrophysik
Externe Organisation(en)
Australian National University
Journal
Communications in Asteroseismology
Band
156
Seiten
13-17
Anzahl der Seiten
5
ISSN
1021-2043
Publikationsdatum
2008
Peer-reviewed
Ja
ÖFOS 2012
103003 Astronomie
Link zum Portal
https://ucrisportal.univie.ac.at/de/publications/46a1c0d1-9502-45d8-ba14-8e68f692bfa3