期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 396, 期 3, 页码 1460-1472出版社
WILEY-BLACKWELL PUBLISHING, INC
DOI: 10.1111/j.1365-2966.2009.14790.x
关键词
stars: individual: 12 Lac; stars: interiors; stars: oscillations
资金
- Research Council of Leuven University [GOA/2008/04]
- Austrian Fonds zur Forderung der wissenschaftlichen Forschung [R12-N02, P18339-N08]
We present the results of a spectroscopic multisite campaign for the beta Cephei star 12 ( DD) Lacertae. Our study is based on more than thousand high-resolution high S/N spectra gathered with eight different telescopes in a time span of 11 months. In addition, we make use of numerous archival spectroscopic measurements. We confirm 10 independent frequencies recently discovered from photometry, as well as harmonics and combination frequencies. In particular, the slowly pulsating B-stars (SPB)-like g-mode with frequency 0.3428 d(-1) reported before is detected in our spectroscopy. We identify the four main modes as (l(1), m(1)) = (1, 1), (l(2), m(2)) = (0, 0), (l(3), m(3)) = (1, 0) and (l(4), m(4)) = (2, 1) for f(1) = 5.178964 d(-1), f(2) = 5.334224 d(-1), f(3) = 5.066316 d(-1) and f(4) = 5.490133 d(-1), respectively. Our seismic modelling shows that f(2) is likely the radial first overtone and that the core overshooting parameter alpha(ov) is lower than 0.4 local pressure scale heights.
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