PL EN


Preferencje help
Widoczny [Schowaj] Abstrakt
Liczba wyników
Tytuł artykułu

Mt. Suhora Survey - Searching for Pulsating M Dwarfs. I

Wybrane pełne teksty z tego czasopisma
Identyfikatory
Warianty tytułu
Języki publikacji
EN
Abstrakty
EN
We present the first results of our M dwarf survey in search for stellar pulsation in low mass main sequence stars. Theoretical calculations predict that ε mechanism might drive a fundamental radial mode in these stars and therefore pulsations could be observed photometrically. Although M dwarfs are known for their flare and spot activity they have not yet been the subject of dedicated time-series surveys for pulsation. In this work we include the light curves and amplitude spectra of 46 M dwarfs, which have been observed during the first two years of our survey. We did not detect any pulsations yet. As a by-product of our search, we describe the light curves of some flare M dwarfs. The survey will last for two more years and during that period more than a hundred of M0-M4 type main sequence stars will be observed.
Czasopismo
Rocznik
Strony
37--58
Opis fizyczny
Bibliogr. 15 poz., rys., tab., wykr.
Twórcy
autor
  • Mt. Suhora Observatory of the Pedagogical University, ul. Podchorążych 2, 30-084 Cracow, Poland
  • Iowa State University, 12 Physics Hall, Ames, IA 50011, USA
autor
  • Mt. Suhora Observatory of the Pedagogical University, ul. Podchorążych 2, 30-084 Cracow, Poland
  • Mt. Suhora Observatory of the Pedagogical University, ul. Podchorążych 2, 30-084 Cracow, Poland
  • Instituto de Astronomia - Universidad Nacional Autónoma de México, Ap. P. 877, Ensenada, BC 22860, Mexico
  • Iowa State University, 12 Physics Hall, Ames, IA 50011, USA
autor
  • Mt. Suhora Observatory of the Pedagogical University, ul. Podchorążych 2, 30-084 Cracow, Poland
  • University of Western Cape, Physics Department, Cape Town 7535, South Africa
  • Missouri State University, Department of Physics, Astronomy, and Materials Science, 901 S. National Av., Springfield, MO 65897, USA
autor
  • Missouri State University, Department of Physics, Astronomy, and Materials Science, 901 S. National Av., Springfield, MO 65897, USA
Bibliografia
  • Baraffe, I., and Chabrier, G. 1996, ApJ, 461, L51.
  • Berger, D.H., et al. 2006, ApJ, 644, 475.
  • Chabrier, G., and Baraffe, I. 1997, A&A, 327, 1039.
  • Chabrier, G., and Baraffe, I. 2000, Ann. Rev. Astron. Astrophys., 38, 337.
  • Cody, A.N., and Hillenbrand, L. 2010, ApJS, 191, 389.
  • Delfosse, X., et al. 2004, in: “Spectroscopically and Spatially Resolving the Components of the Close Binary Stars” ASP Conference Series, vol. 318, 166.
  • Gliese, W., and Jahreiss, H. 1979, A&AS, 38, 423.
  • Henry, J.W., et al. 2006, AJ, 132, 2360.
  • Hertzsprung, E. 1924, Bulletin of the Astronomical Institutes of the Netherlands, 2, 87.
  • Hillenbrand, L.A., and White, R.J. 2004, ApJ, 604, 741.
  • Kawaler, S.D. 1988, ApJ, 334, 220.
  • López-Morales, M., and Ribas, I. 2005, ApJ, 631, 1120.
  • Palla, F., and Baraffe, I. 2005, A&A, 432, L57.
  • Stetson, P.B. 1987, PASP, 99, 191.
  • Unno, W., Osaki, Y., Ando, H., Saio, H., and Shibahashi, H. 1989, “Nonradial Oscillations of Stars”, (2nd ed.), Tokyo: U. Tokyo Press.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-e4092726-f6e5-4b63-afaf-2b7e0e911f63
JavaScript jest wyłączony w Twojej przeglądarce internetowej. Włącz go, a następnie odśwież stronę, aby móc w pełni z niej korzystać.