Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/5555
Title: A spectroscopic study of the hybrid pulsator Gamma Pegasi
Authors: Pandey, C. P
Morel, T
Briquet, M
Jayakumar, K
Bisht, S
Sanwal, B. B
Issue Date: Feb-2011
Publisher: Austrian Academy of Sciences Press
Citation: Communications in Asteroseismology, Vol. 162, pp. 21-49
Abstract: The recent detection of both pressure and high-order gravity modes in the clas- sical B-type pulsator γ Pegasi offers promising prospects for probing its internal structure through seismic studies. To aid further modelling of this star, we present the results of a detailed NLTE abundance analysis based on a large number of time-resolved, high-quality spectra. A chemical composition typical of nearby B-type stars is found. The hybrid nature of this star is consistent with its location in the overlapping region of the instability strips for β Cephei and slowly pulsating B stars computed using OP opacity tables, although OPAL cal- culations may also be compatible with the observations once the uncertainties in the stellar parameters and the current limitations of the stability calcula- tions are taken into account. The two known frequencies f1 = 6.58974 and f2 = 0.68241 d−1 are detected in the spectroscopic time series. A mode iden- tification is attempted for the low-frequency signal, which can be associated to a high-order g-mode. Finally, we re-assess the binary status of γ Peg and find no evidence for variations that can be ascribed to orbital motion, contrary to previous claims in the literature.
URI: http://hdl.handle.net/2248/5555
???metadata.dc.rights???: © Austrian Academy of Sciences Press
???metadata.dc.relation.uri???: http://www.univie.ac.at/tops/CoAst/archive/Cia162.pdf
http://adsabs.harvard.edu/abs/2011CoAst.162...21P
Appears in Collections:IIAP Publications

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