Two-site CCD observations and spectroscopy of HD 207331: a new Scuti variable in Cygnus
arXiv:1007.2048 · doi:10.1016/j.newast.2010.05.005
Abstract
The results of an observational campaign on the new Scuti pulsator \astrobj{HD~207331} are reported. The star was observed photometrically from August 26 to September 2, 2009 from the Observatorio San Pedro Mártir (0.84-m telescope, Mexico) and the Observatorio del Teide (0.80-m telescope, Spain). An overall run of 53.8 h of useful data was collected from the two sites. Four oscillation frequencies for \astrobj{HD~207331} have been found above a 99\% confidence level. These results confirm the multiperiodic pulsation nature of the star suggested in previous observations with sparse data. Spectroscopic observations carried out in 2009 allowed us to derive its spectral type and luminosity class as well as to estimate its rotation rate. A simple comparison with models is performed.
arXiv comment6 pages, 5 figures, 3 tables, New Astronomy 15 (2010) 712-716
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