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

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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2010-11-22

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