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The Gravitational Potential in Close Binary Star Systems
20th International Symposium on High-Performance Computing in an Advanced Collaborative Environment (HPCS'06), 2006The gravitational potential for close binary systems is usually calculated assuming both stars to be point masses. Deupree and Karakas recently examined the internal structure of both members of a binary system under the assumption that the gravitational potential for each member is the gravitational potential produced by its own mass distribution and ...
Robert G. Deupree, Patrick Rogers
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Rotation in Close Binary Stars
Highlights of Astronomy, 1980In binary stars of short period, axial rotation of the components tends to be synchronized with the orbital revolution. Rotation of B. and A stars is therefore slowed down, while for the later-type stars, it is accelerated. This latter fact probably contributes to the phenomenon of the RS CVn stars.
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, 2019
Close binaries suppress the formation of circumstellar (S-type) planets and therefore significantly bias the inferred planet occurrence rates and statistical trends.
M. Moe, K. Kratter
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Close binaries suppress the formation of circumstellar (S-type) planets and therefore significantly bias the inferred planet occurrence rates and statistical trends.
M. Moe, K. Kratter
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An Introduction to Close Binary Stars
2001Binary systems of stars are as common as single stars. They are of fundamental importance because they allow stellar masses, radii and luminosities to be measured directly, and explain a host of diverse and energetic phenomena including X-ray binaries, cataclysmic variables, novae, symbiotic stars, and some types of supernovae.
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Close Binary Stars and Their Significance for the Theory of Stellar Evolution
Uspekhi Fizicheskih Nauk, 1972CONTENT 1. Introduction 786 2. Binary Stars 788 3. Orbit Variations of the Close Pair 790 4. Evolution of Stars in Close Binary Systems 792 5. Successes and Failures of Theory 795 6. Novae and Binary Stars 796 7. Black Holes 797 8.
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Close-Binary Stars in Planetary Nebulae
2019It is now clear, after many years of heated debate, that a significant fraction of planetary nebulae are the product of close-binary evolution. In this chapter, we present the history of the field and some of the obstacles that have hindered progress - including detailed descriptions of the techniques employed and their limitations.
Henri M. J. Boffin, David Jones
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Interactive stars: Normal and compact stars in close binaries
AIP Conference Proceedings, 1990The missions planned for the 1990’s will greatly expand our knowledge of close binary systems and the physical phenomena that can be studied in a member of a close binary, from stellar active regions to the highest density black hole candidates known.
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Close Binary Stars. VIII: Close Binary Star Systems in the Late Stages of Evolution
Astronomy Reports, 2022openaire +1 more source
Close Binary Stars. VII: On the Evolution of Close Binary Systems
Astronomy Reports, 2022openaire +1 more source