Reference : Asteroseismology of the new multiperiodic gamma Dor variable HD 239276
Scientific journals : Article
Physical, chemical, mathematical & earth Sciences : Space science, astronomy & astrophysics
http://hdl.handle.net/2268/75398
Asteroseismology of the new multiperiodic gamma Dor variable HD 239276
English
Rodríguez, E. [Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain]
Costa, V. [Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain]
Zhou, A*-Y [National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, PR China]
Grigahcène, A. [CRAAG, Algiers Observatory, BP 63 Bouzareah 16340, Algiers, Algeria]
Dupret, Marc-Antoine [Université de Liège - ULiège > Département d'astrophys., géophysique et océanographie (AGO) > Astrophysique stellaire théorique >]
Suárez, J. C. [Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain; LESIA, Observatoire de Paris-Meudon, UMR 8109, 92190 Meudon, France]
Moya, A. [Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain; LESIA, Observatoire de Paris-Meudon, UMR 8109, 92190 Meudon, France]
López-González, M. J. [Instituto de Astrofísica de Andalucía, CSIC, PO Box 3004, 18080 Granada, Spain]
Wei, J*-Y [National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, PR China]
Fan, Y. [National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, PR China]
1-Sep-2006
Astronomy and Astrophysics
EDP Sciences
456
261-268
Yes (verified by ORBi)
International
0004-6361
1432-0746
Les Ulis
France
[en] stars: variables: general ; stars: individual: HD 239276 ; stars: oscillations ; techniques: photometric
[en] The variability of HD 239276 was suspected photometrically nearly twenty years ago, but was confirmed with new observations obtained in 2001 during a two-site photometric campaign carried out from Spain, in uvbybeta Strömgren-Crawford photometry, and China, using the Johnson V filter. Two low-dispersion spectra were also collected. The results establish this star as a new multiperiodic gamma Dor-type pulsator with deficiency in metallicity. Its possible lambda Boo nature is discussed. The frequency analysis shows three pulsational frequencies as significant, but some more are probably present among the residuals. The method based on phase shifts and amplitude ratios in multicolour photometry is used to identify the excited modes with non-adiabatic time-dependent convection models. A very good agreement between the theoretical and observed amplitude ratios is obtained and the two main modes are identified as l=1 modes. Nevertheless, our results do not allow us to discriminate between a solar abundance and a metal deficient nature for this star. The frequency ratio method is further used for the identification of the modes. The results suggest low metallicity for this star, but a lambda Boo nature may be not ruled out.
http://hdl.handle.net/2268/75398
10.1051/0004-6361:20065211
http://adsabs.harvard.edu/abs/2006A%26A...456..261R

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