Hostname: page-component-cd9895bd7-8ctnn Total loading time: 0 Render date: 2024-12-25T17:53:11.240Z Has data issue: false hasContentIssue false
  • English
  • Français

Physics of Eclipsing Binaries: Heartbeat Stars and Tidally Induced Pulsations

Published online by Cambridge University Press:  25 February 2014

K. Hambleton ,
P. Degroote ,
K. Conroy ,
S. Bloemen ,
D. Kurtz ,
S.E. Thompson ,
J. Fuller ,
J. Giammarco ,
H. Pablo  and
A. Prša
K. Hambleton
Affiliation:
Department of Astrophysics and Planetary Science, Villanova University, 800 Lancaster Ave., Villanova, PA 19085, USA Jeremiah Horrocks Institute, University of Central Lancashire, Preston, PR1 2HE, UK
P. Degroote
Affiliation:
Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
K. Conroy
Affiliation:
Department of Physics and Astronomy, Vanderbilt University, VU Station B 1807, Nashville, TN 37235, USA
S. Bloemen
Affiliation:
Instituut voor Sterrenkunde, KU Leuven, Celestijnenlaan 200D, 3001 Leuven, Belgium
D. Kurtz
Affiliation:
Jeremiah Horrocks Institute, University of Central Lancashire, Preston, PR1 2HE, UK
S.E. Thompson
Affiliation:
NASA Ames Research Center, Moffett Field, CA 94035, USA
J. Fuller
Affiliation:
California Institute of Technology, TAPIR 350-17, 1200 E. California Boulevard, Pasadena, CA 91125-0001, USA
J. Giammarco
Affiliation:
Department of Astronomy and Physics, Eastern University, Saint Davids, PA 19087, USA
H. Pablo
Affiliation:
Département de Physique, Université de Montréal, CP 6128, Succursale Centre-Ville, Montreal, QC, H3C 3J7, Canada
A. Prša
Affiliation:
Department of Astrophysics and Planetary Science, Villanova University, 800 Lancaster Ave., Villanova, PA 19085, USA
Get access

Abstract

Heartbeat stars are a relatively new class of eccentric ellipsoidal variable first discovered by Kepler. An overview of the current field is given with details of some of the interesting objects identified in our current Kepler sample of 135 heartbeats stars. Three objects that have recently been or are undergoing detailed study are described along with suggestions for further avenues of research. We conclude by discussing why heartbeat stars are an interesting new tool to study tidally induced pulsations and orbital dynamics.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 64: Setting a New Standard in the Analysis of Binary Stars , 2013 , pp. 285 - 294
Copyright
© EAS, EDP Sciences, 2014

Access options

Get access to the full version of this content by using one of the access options below. (Log in options will check for institutional or personal access. Content may require purchase if you do not have access.)

References

Burkart, J., Quataert, E., Arras, P., & Weinberg, N.N., 2011 [arXiv]
Derekas, A., Kiss, L.L., Borkovits, T., et al., 2011, Science, 332, 216CrossRef
Espinosa Lara, F., & Rieutord, M., 2012, A&A, 547, A32
Fuller, J., & Lai, D., 2011, MNRAS, 420, 3126CrossRef
Gies, D.R., Williams, S.J., Matson, R.A., et al., 2012, AJ, 143, 137CrossRef
Hambleton, K., Kurtz, D.W., Prša, A., et al., 2013, MNRAS, 434, 925CrossRef
Hut, P., 1981, A&A, 99, 126
Kumar, P., Ao, C.O., & Quataert, E.J., 1995, ApJ, 449, 294CrossRef
Kurtz, D.W., 1976, ApJS, 32, 651CrossRef
Lucy, L.B., 1967, Zeit. Astrof., 65, 89
Nicholls, C.P., & Wood, P.R., 2012, MNRAS, 421, 2616CrossRef
Papaloizou, J., & Pringle, J.E., 1981, MNRAS, 196, 371CrossRef
Prša, A., & Zwitter, T., 2005, ApJ, 628, 426CrossRef
Shibahashi, H., & Kurtz, D.W., 2012, MNRAS, 422, 738CrossRef
Thompson, S.E., Everett, M., Mullally, F., et al., 2012, ApJ, 753, 86CrossRef
Welsh, W.F., Orosz, J.A., Aerts, C., et al., 2011, ApJS, 197, 4CrossRef
Willems, B., & Claret, A., 2005, ASP Conf. Ser., 333, 52
Wilson, R.E., 1979, ApJ, 234, 1054CrossRef