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Abstrakty
EN
We performed new observations of an ultra-fast rotator of the spectral class K - the LO Peg star - in SAO RAS in 2014 and in Zvenigorod Observatory of INASAN in 2015. The light curves were used to build the maps of temperature inhomogeneities on the LO Peg surface in order to determine the longitudes corresponding to the location of active regions. The obtained measurements suggest the ongoing evolution of movements of active regions and probably the cyclic character of such movements. According to our estimations, the area of the star surface covered with spots decreases and by now it reached 14% of the total visible area of its surface. New observations of the star in V filter allowed us to specify LO Peg long-term variability cycles. Based on spectropolarimetric observations of LO Peg the null result for measurements of mean longitudinal component of magnetic field is obtained.
Słowa kluczowe
Czasopismo
Rocznik
Strony
381--390
Opis fizyczny
Bibliogr. 24 poz., rys.
Twórcy
  • Institute of Astronomy of Russian Academy of Sciences, Pyatnitskaya, 48, 119017 Moscow, Russia
autor
  • Institute of Astronomy of Russian Academy of Sciences, Pyatnitskaya, 48, 119017 Moscow, Russia
  • Lomonosov Moscow State University, Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russia
autor
  • Special Astrophysical Observatory of Russian Academy of Sciences, Nizhniy Arkhyz, Russia
  • Kazan Federal University, 18 Kremlevskaya st., Kazan, 420008 Russia
autor
  • Special Astrophysical Observatory of Russian Academy of Sciences, Nizhniy Arkhyz, Russia
  • Kazan Federal University, 18 Kremlevskaya st., Kazan, 420008 Russia
  • Lomonosov Moscow State University, Sternberg Astronomical Institute, Universitetskii pr. 13, Moscow 119992, Russia
  • Kazan Federal University, 18 Kremlevskaya st., Kazan, 420008 Russia
autor
  • Precision Systems & Instruments Corp., 53 Aviamotornaya st., Moscow, 111024 Russia
autor
  • Precision Systems & Instruments Corp., 53 Aviamotornaya st., Moscow, 111024 Russia
  • Precision Systems & Instruments Corp., 53 Aviamotornaya st., Moscow, 111024 Russia
autor
  • Precision Systems & Instruments Corp., 53 Aviamotornaya st., Moscow, 111024 Russia
autor
  • Precision Systems & Instruments Corp., 53 Aviamotornaya st., Moscow, 111024 Russia
autor
  • Kazan Federal University, 18 Kremlevskaya st., Kazan, 420008 Russia
  • Special Astrophysical Observatory of Russian Academy of Sciences, Nizhniy Arkhyz, Russia
  • Special Astrophysical Observatory of Russian Academy of Sciences, Nizhniy Arkhyz, Russia
  • Special Astrophysical Observatory of Russian Academy of Sciences, Nizhniy Arkhyz, Russia
autor
  • Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital 263002, India
autor
  • Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital 263002, India
autor
  • Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital 263002, India
autor
  • Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital 263002, India
autor
  • Aryabhatta Research Institute of Observational Sciences (ARIES), Manora Peak, Nainital 263002, India
Bibliografia
  • Bagnulo, S., Szeifert, T., Wade, G.A., Landstreet, J.D., and Mathys, G. 2002, A&A, 389, 191.
  • Barnes, J.R., Collier Cameron, A., Lister, T.A., Pointer, G.R., and Still, M.D. 2005, MNRAS, 356, 1501.
  • Beskin, G., et al. 2010, Physics Uspekhi, 53, 406.
  • Biryukov, A., Beskin, G., Karpov, S., Bondar, S., Ivanov, E., Katkova, E., Perkov, A., and Sasyuk, V. 2015, Baltic Astronomy, 24, 100.
  • Chountonov, G.A. 2004, in: “Proceedings of the International Meeting on Magnetic Stars”, Eds. Yu. Glagolevskij, I. Romanyuk.286
  • Dal, H.A., and Tas, G. 2003, IBVS, 5390.
  • Jaervinen, S.P., Korhonen, H., Berdyugina, S.V., Ilyin, I., Strassmeier, K.G., Weber, M., Savanov, I., and Tuominen, I. 2008, A&A, 488, 1047.
  • Jeffries, R.D., Byrne, P.B., Doyle, J.G., Anders, G.J., James, D.J., and Lanzafame, A.C. 1994, MNRAS, 270, 153.
  • Karmakar, S., et al. 2016, MNRAS, 459, 3112.
  • Kudryavtsev, D.O. 2000, Baltic Astronomy, 9, 649.
  • Landstreet, J.D. 1982, ApJ, 258, 639.
  • Lister T.A., Collier Cameron A., and Bartus J. 1999, MNRAS, 307, 685.
  • López-Santiago, J., Montes, D., Crespo-Chacón, I., and Fernández-Figueroa, M.J. 2006, ApJ, 643, 1160.
  • Pandey J.C., Singh K.P., Drake S.A., and Sagar, R. 2005, AJ, 130, 1231.
  • Piluso N., Lanza, A.F., Pagano, I., Lanzafame, A.C., and Donati, J.-F. 2008, MNRAS, 387, 237.
  • Puzin, V.B., Savanov, I.S., Romanyuk, I.I., Semenko, E.A., and Dmitrienko, E.S. 2014, Astrophysical Bulletin, 69, 321.
  • Robb R.M., and Cardinal R.D. 1995, IBVS, 4221.
  • Savanov I.S., and Strassmeier K.G. 2008, Astron. Nachr., 329, 364.
  • Savanov, I.S 2010, Astronomy Reports, 54, 1125.
  • Savanov, I.S., and Dmitrienko, E.S. 2011, Astronomy Reports, 55, 437.
  • Savanov, I.S., Romanyuk, I.I., Semenko, E.A., and Dmitrienko, E.S. 2011, Astronomy Reports, 55, 111.
  • Savanov, I.S., Romaniuk, I.I., Semenko, E.A., and Dmitrienko, E.S. 2013, Astronomy Reports, 57, 751.
  • Tas, G. 2011, Astron. Nachr., 332, 57.
  • Zuckerman, B., Song I., and Bessell, M.S. 2004, ApJ, 613, L65.
Uwagi
Opracowanie rekordu w ramach umowy 509/P-DUN/2018 ze środków MNiSW przeznaczonych na działalność upowszechniającą naukę (2019).
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-eba22cf0-d666-44fa-9576-d42327eac2eb
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