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Download e-book for kindle: Interacting Binaries by R. F. Griffin (auth.), P. P. Eggleton, J. E. Pringle (eds.)

By R. F. Griffin (auth.), P. P. Eggleton, J. E. Pringle (eds.)

ISBN-10: 9400953372

ISBN-13: 9789400953376

ISBN-10: 940108856X

ISBN-13: 9789401088565

Peter P. Eggleton and James E. Pringle Institute of Astronomy Madingley highway Cambridge England The 1970's could be defined, looking back, because the "Decade of the shut Binary". interesting observations with new know-how, mixed with classical paintings, either observational and theoretical, confident the astronomical global that binary interplay of varied forms isn't just attention-grabbing yet universal. certainly, via 1975 virtually something strange had a superb opportunity of being interpreted as because of binary interplay. yet astronomers are seldom crushed by means of hypothesis, even their very own, and good observational paintings has proven or refuted such hypothesis, with out regard to its plausibility. for example, binarity has been discovered the place it used to be maybe least anticipated, in Barium stars, and refuted the place it may possibly so much quite be anticipated, in Wolf-Rayets. regrettably, many different sessions of capability binaries stay with no the clearest facts of binarity, for example Be stars, symbiotics and blue stragglers. This complex examine Institute was once held to commemorate John Whelan (1945-1981), whose medical occupation, unfortunately reduce brief in its major, did a lot to additional the cautious examine, theoretical and observational, of shut binaries, in addition to to motivate the spirit of overseas friendship and collaboration. His personal pursuits lined a better box, yet "Interacting Binaries" appeared a cheap limit. We submit right here 15 assessment talks, which nonetheless don't hide the complete subject, even though they vary widely.

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Emissions still wait to be done. c) Transition region emission seems to be very similar to that of other very active stars: it behaves as a continuation of trends "saturated" at about 3 days with very little dependence on the spectral type. d) Coronal activity of contact binaries, as measured by the X-ray emission, is smaller by a factor of a few than in normal, most active, non-contact stars. The very strong under-activity of F-type contact systems previously noticed is less striking when it is realized that non-contact systems of earlier spectral types also show a sharp drop in activity.

5 7"9 NY I 01 en I I SilY II AW UMa OUL1~200--~-------1-4~00~--~----~16~0~0--------~18~00~----~ ACAl 0 . 2 'III el I 7e U 0\ t ... 1 Hen SilV I M Sin II 01 - 'g )( I -< 0 R 1200 1400 1600 1800 A('~) Fi gur e 9 . Low resolution IUE spectra of AW UMa (upper panel) and SW Lac ( l ower panel ) revealing strong emi s sion lines whi ch or igi nat e in the transition region. Notice that in spite of very di ffe r ent continuum spectra (s pect ral type of AW UMa is FO- 2 ; spectral t ype o f SW Lac is G6 - 8) , the line strengths are ve r y s i mi l ar .

1982, ESo Messanger, 28, 15. Astrophys. 70, 91. Astrophys. 80, 287. Space Sci. 78, 401. , 109, 17. , 133, 117. Vilhu, o. , 127, 5. , 274, 794. , 215, 851. Soc. 156, 115. E. , 1976. , 48, 349. E. , 182, 539. J. ), 199, L63. , 208, 414. Zirin, H. , 259, 719. OBSERVATIONAL EVIDENCE FOR THE EVOLUTION OF CONTACT BINARY STARS Stefan W. Mochnacki David Dunlap Observatory University of Toronto Ontario, Canada ABSTRACT This paper reviews data relevant to the evolution of contact binary stars. Statistics, photometric surveys, period changes and the results of light curve fitting are reviewed.

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Interacting Binaries by R. F. Griffin (auth.), P. P. Eggleton, J. E. Pringle (eds.)

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