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2007MNRAS.378.1049R - Mon. Not. R. Astron. Soc., 378, 1049-1063 (2007/July-1)
Resolving the pulsations of subdwarf B stars: HS 0039+4302, HS 0444+0458 and an examination of the group properties of resolved pulsators.
REED M.D., TERNDRUP D.M., ZHOU A.-Y., UNTERBORN C.T., AN D. and EGGEN J.R.
Abstract (from CDS):
Including the two stars in this paper, 23 pulsating sdB stars have received follow-up observations designed to decipher their pulsation spectra. It is worth an examination of what has been detected. We compare and contrast the frequency content in terms of richness and range and the amplitudes with regard to variability and diversity. We use this information to examine observational correlations with the proposed κ pulsation mechanism as well as alternative theories.
Abstract Copyright: 2007 The Authors. Journal compilation © 2007 RAS
Journal keyword(s): stars: individual: HS 0039+4302 - stars: individual: HS 0444+0857 (read: HS 0444+0458) - stars: oscillations - subdwarfs - stars: variables: others
CDS comments: In Keywords : HS 0444+0857 is a misprint for HS 0444+0458, In Table 1 : PG 0014+182 is a misprint for PG 0014+067.
Simbad objects: 24
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