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Insights into the Pulsational Behaviour of δ Sct Stars

Published online by Cambridge University Press:  12 April 2016

L. Mantegazza
Affiliation:
Universitá di Pavia, Dipartimento di Fisica Nucleare e Teorica, Via Bassi 6, 27100 Pavia, Italy
E. Poretti
Affiliation:
Osservatorio di Brera, Via E. Bianchi 46, 22055 Merate, Italy

Extract

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Extensive photometric monitoring of bright δ Scuti stars, made in the last years, allowed us to get reliable frequency determinations also in very complicated cases. Table 1 gives a full description of our photometric targets. Recently, we realized that combining photometry with simultaneous high resolution spectroscopy, in order to study line profile variations, offers the possibility to perform a much more reliable mode identification. Hence, the photometric runs of FG Vir, X Cae, HD 2724 were paired with spectroscopic ones obtained at the Coudé Auxiliary Telescope (ESO, La Silla, Chile). The stellar spectra are centred at 4508 Å and they cover a range of 37.6 Å; the resolving power is about 50000-60000 and the linear dispersion is 2.4 Å/mm.

Type
Part 2. Poster Papers
Copyright
Copyright © Astronomical Society of the Pacific 1995