"INTER-LONGITUDE ASTRONOMY" (ILA) PROJECT: CURRENT HIGHLIGHTS AND PERSPECTIVES. I. MAGNETIC VS. NON-MAGNETIC INTERACTING BINARY STARS

Автор(и)

  • I. L. Andronov Department "High and Applied Mathematics", Odessa National Maritime University, Україна
  • K. A. Antoniuk Crimean Astrophysical Observatory, Nauchny, Україна
  • A. V. Baklanov Crimean Astrophysical Observatory, Nauchny, Україна
  • V. V. Breus Department "High and Applied Mathematics", Odessa National Maritime University, Україна
  • V. Burwitz Max-Planck Institut fur Extra-Terrestische Physik, Garching, Німеччина
  • L. L. Chinarova Department of Astronomy and Research Institute "Astronomical Observatory", Odessa National University, Україна
  • D. Chochol Astronomical Institute of the Slovak Academy of Sciences, Stara Lesna,, Словаччина
  • P. A. Dubovsky Vihorlat Astronomical Observatory, Humenne, Словаччина
  • W. Han Korea Astronomy and Space Science Institute, Daejeon, Південна Корея
  • T. Hegedus Baja Astronomical Observatory, Baja, Угорщина
  • A. Henden American Association of Variable Stars Observers, Harvard, США
  • L. Hric Astronomical Institute of the Slovak Academy of Sciences, Stara Lesna, Словаччина
  • Chun-Hwey Kim University Observatory, Chungbuk National University, Cheongju, Південна Корея
  • Yonggi Kim University Observatory, Chungbuk National University, Cheongju, Південна Корея
  • S. V. Kolesnikov Department of Astronomy and Research Institute "Astronomical Observatory", Odessa National University, Україна
  • I. Kudzej Vihorlat Astronomical Observatory, Humenne, Словаччина
  • A. Liakos Department of Astrophysics, Astronomy and Mechanics, University of Athens, Греція
  • P. G. Niarchos Department of Astrophysics, Astronomy and Mechanics, University of Athens, Греція
  • A. Oksanen Hankasalmi Observatory, Hankasalmi, Фінляндія
  • L. Patkos Konkoly Observatory, Hungarian Academy of Sciences, Budapest, Угорщина
  • K. Petrik Astronomical Observatory, Hlohovec, Словаччина
  • N. V. Pit' Crimean Astrophysical Observatory, Nauchny, Україна
  • N. M. Shakhovskoy Crimean Astrophysical Observatory, Nauchny, Україна
  • N. A. Virnina Department "High and Applied Mathematics", Odessa National Maritime University, Україна
  • J. Yoon University Observatory, Chungbuk National University, Cheongju, Південна Корея
  • S. Zola Astronomical Observatory, Jagiellonian University, Cracow, Польща

DOI:

https://doi.org/10.18524/1810-4215.2010.23.84023

Ключові слова:

Variable stars, cataclysmic, pulsating, eclipsing, interacting binary

Анотація

We present a review of highlights of our photometric and photo-polarimetric monitoring and mathematical modeling of interacting binary stars of different types classical, asynchronous, intermedi ate polars with 25 timescales corresponding to differ ent physical mechanisms and their combinations (part "Polar"); negative and positive superhumpers in nova-like and dwarf novae stars ("Superhumper"); symbiotic ("Symbiosis"); eclipsing variables with and without ev idence for a current mass transfer ("Eclipser") with a special emphasis on systems with a direct impact of the stream into the gainor star's atmosphere, which we propose to call "Impactors", or V361 Lyr-type stars. Other parts of the ILA project are "Stellar Bell" (pul sating variables of different types and periods - M, SR, RV Tau, RR Lyr, Delta Sct) and "New Variable". 

Посилання

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Опубліковано

2010-11-22

Номер

Том 23 (2010)

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Відповідно Закону України про авторське право і суміжні права N 3792-XII від 23 грудня 1993 року