MOST observations of the Herbig Ae δ-Scuti star HD 34282

被引:12
作者
Casey, M. P. [1 ]
Zwintz, K. [2 ]
Guenther, D. B. [1 ]
Weiss, W. W. [2 ]
Amado, P. J. [3 ]
Diaz-Fraile, D. [3 ]
Rodriguez, E. [3 ]
Kuschnig, R. [2 ]
Matthews, J. M. [4 ]
Moffat, A. F. J. [5 ]
Rowe, J. F. [6 ]
Rucinski, S. M. [7 ]
Sasselov, D. [8 ]
机构
[1] St Marys Univ, Dept Phys & Astron, Inst Computat Astrophys, Halifax, NS B3H 3C3, Canada
[2] Univ Vienna, Inst Astron, A-1180 Vienna, Austria
[3] CSIC, Inst Astrofis Andalucia, E-18080 Granada, Spain
[4] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[5] Univ Montreal, Dept Phys, Montreal, PQ H3C 3J7, Canada
[6] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[7] Univ Toronto, Dept Astron & Astrophys, Toronto, ON M5S 3H4, Canada
[8] Harvard Smithsonian Ctr Astrophys, Cambridge, MA 02138 USA
基金
加拿大自然科学与工程研究理事会; 奥地利科学基金会;
关键词
asteroseismology; techniques: photometric; stars: individual: HD 34282; stars: pre-main sequence; stars: variables: delta Scuti; MAIN-SEQUENCE STARS; SPECTRAL CLASSIFICATION; FREQUENCY; PHOTOMETRY; SATELLITE; CATALOG; SPACE; MODES; SUN;
D O I
10.1093/mnras/sts241
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Microvariability and Oscillations of STars (MOST) observations and model analysis of the Herbig Ae star HD 34282 (V1366 Ori) reveal delta Scuti pulsations. 22 frequencies are observed, 10 of which confirm those previously identified by Amado et al. and 12 of which are newly discovered in this work. We show that the weighted-average frequency in each group fits the radial p-mode frequencies of viable models. We argue that the observed pulsation spectrum extends just to the edge to the acoustic cut-off frequency and shows that this is also consistent with our best-fitting models.
引用
收藏
页码:2596 / 2604
页数:9
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