The multiple frequencies of the δ Scuti star V350 Peg^*

¹ Grup d'Estudis Astronomics, Apdo. 9481, 08080 Barcelona, Spain e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
² Vereniging Voor Sterrenkunde, Belgium e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
³ Koninklijke Sterrenwacht van België, Ringlaan 3, 1180 Brussel, Belgium e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.
⁴ Esteve Duran Observatory Foundation, Montseny 46 – Urb. El Montanya, 08553 Seva, Spain e-mail: This email address is being protected from spambots. You need JavaScript enabled to view it.

Corresponding author: P. Lampens, This email address is being protected from spambots. You need JavaScript enabled to view it.

Received: 5 June 2002
Accepted: 5 August 2002

Abstract

V350 Peg is a δ Scuti star discovered by Hipparcos (ESA [CITE]). During 35 nights between July 1997 and December 2001 some 7500 CCD V observations were acquired at the Monegrillo and Esteve Duran observatories in Spain. The new data show that this star pulsates in a close doublet of frequencies separated by 0.17 c/d (%) with similar amplitudes. More frequencies are excited but cannot be identified with certainty. The period as listed in the Hipparcos Catalogue is not confirmed.