Open AccessThe EC 14026 stars – VII. PG 1605+072, a star with many pulsation modes
Author(s) -
C. Koen,
D. O’Donoghue,
D. Kilkenny,
A. E. Lynas-Gray,
F. Marang,
F. van Wyk
Publication year - 1998
Publication title -
monthly notices of the royal astronomical society
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.058
H-Index - 383
eISSN - 1365-2966
pISSN - 0035-8711
DOI - 10.1046/j.1365-8711.1998.01435.x
Subject(s) - physics , stars , astrophysics , star (game theory) , amplitude , harmonics , variable star , range (aeronautics) , astronomy , optics , materials science , quantum mechanics , voltage , composite material
We report the discovery of large‐amplitude (∼0.25 mag) pulsations in the bright ( V =12.8) sdB star, PG 1605+072. The dominant period is 480 s, but more than 20 periods were present on at least three separate occasions. Frequency analysis of the complete data set yields more than 30 periods. A few of these are harmonics or linear combinations of the strongest modes. Excluding the latter, the periods span a range of almost 400 s, which contrasts with the typical range <20 s for most other EC 14026 stars. Analysis of multicolour photometry limited any cool companion to being a main‐sequence star of type M0 or later. Balmer line profile fitting yielded an effective temperature of 32 100±1000 K and a log g of 5.25±0.10, significantly smaller than in the other stars of the EC 14026 class, and possibly indicative of a more evolved state. The lower gravity is probably responsible for the fact that the pulsation periods and amplitudes are respectively much longer and larger than in other stars of the class. This star is an obvious target for asteroseismological investigation using a multilongitude photometric campaign.