By Cecilia Payne-Gaposchkin (auth.), M. Friedjung (eds.)
Michael Friedjung even though identified because antiquity, novae are nonetheless poorly below stood and current many difficulties. There has tended to be an absence of conversation among theoreticians and observers and among various faculties of suggestion, despite the advances of contemporary years in convinced instructions (observations of normal novae at minimal and of dwarf novae, thought of the reasons of the explosion, and so forth ••• ). The assembly whose lawsuits are contained during this quantity was once equipped to stimulate a confron tation among different principles and effects. the topic has replaced much considering 1963, while the former overseas assembly was once held. there have been sixty one individuals on the convention from 17 international locations, so very many teams ~oing examine within the box of novae have been represented. The reader will see that the topic has turn into extra actual (we comprehend for example that the binary nature of novae is vital) yet a lot paintings is still performed. there's nonetheless a wide gulf among concept and statement. may possibly he locate right here many new rules for destiny examine! i need to thank the French Centre nationwide de l. a. Recherche Scientifique for offering monetary support. i need to additionally thank the opposite contributors of the medical committee (Profs and Drs bathtub, Mustel, Payne-Gaposchkin, Sparks and Warner) and of the neighborhood committee (Audouze, Mrs Steinberg, Vauclair).
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Additional info for Novae and Related Stars: Proceedings of an International Conference Held by the Institut D’Astrophysique, Paris, France, 7 to 9 September 1976
188, 489. J. Astrophys. 2~337. , 1971a, IAU Colloquium 15, 248. , 1971b, Acta Astronomica-2l, 15. , 1972, Acta Astronomica, 22, 1. , 1976, Paper presente~at the Illinois conference on Novae, Illinois. E. , 90, 189. , 1977, In this volume. , 1974, Astr. & Astrophys. 36, 369. Soc. South Africa, ~, 21. Soc. 170, 219. Warner, B. Soc. 152, 219. , 1976, Nature, 262, 271. ON THE STABILITY OF ACCRETION DISKS MARIO LIVIO and GIORA SHAVIV DEPARTMENT OF PHYSICS AND ASTRONOMY TEL-AVIV UNIVERSITY, RAMAT AVIV, ISRAEL The steady state equilibrium equations for accretion disks are analysed for stability against pressure equilibrated perturbations and stability conditions are derived in the linear approxmation.
In the former case detailed models give a good fit to the observations. Much work remains to be done in the Obvious areas for future research are: latter case. A) Red component structure and mass transfer behaviour. Further work on the linear stability of stars conforming to the Roche potential, extending that of PapaloizDu and Bath (1975), would clearly be worth while. In the case of non-linear models, the inclusion of time-dependent convection (if only schematically) is a priority. Ideally a two dimensional hydrodynamic non-linear study is required.
168, 235. Warner, B. 1975a. , 170, 219. Warner, B. 1975b. , 173, 37 P. Warner, B. J. 1974. , 166, 673. Warner, B. M. 1974. , 94, 116. Warner, B. M. 1973. , 756. Warner, B. E. 1971. , 152, 219. Warner, B. E. 1972a. , 156, 1. Warner, B. E. 1972b. , 156, 297. Warner, B. E. 1972c. , 156, 305. Warner, B. L. 1972. , 159, 101. Warner, B. D. 1975. , 172, 433. Weber, R. 1960. , 44, 275. Wegner, G. 1972. Letters, 12, 219. G. 1966. , 143, 121. O. 1957. , 69, 522. 5. This difference is not understood, but appears to be associated with the accretion disc luminosities rathe r than the properties of the stellar components.