Journal
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume 427, Issue 3, Pages 2512-2522Publisher
WILEY-BLACKWELL
DOI: 10.1111/j.1365-2966.2012.22125.x
Keywords
line: profiles; techniques: spectroscopic; stars: individual: HD12901; stars: oscillations; stars: variables: general
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Funding
- Marsden Fund
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Using multisite spectroscopic data collected from three sites, the frequencies and pulsational modes of the ? Doradus star HD?12901 were identified. A total of six frequencies in the range 12?d-1 were observed, their identifications supported by multiple line-profile measurement techniques and previously published photometry. Five frequencies were of sufficient signal-to-noise ratio for mode identification, and all five displayed similar three-bump standard deviation profiles which were fitted well with (l,m) = (1,1) modes. These fits had reduced ?2 values of less than 18. We propose that this star is an excellent candidate to test models of non-radially pulsating ? Doradus stars as a result of the presence of multiple (1,1) modes.
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