Late Evolution of Close Binaries

1971 ◽  
Vol 168 ◽  
pp. 217 ◽  
Author(s):  
Samuel C. Vila
Keyword(s):  
Close Binaries ◽  
Late Evolution

scholarly journals 35. Stellar Constitution (Constitution Des Étoiles)

1991 ◽  
Vol 21 (1) ◽  
pp. 421-437
Keyword(s):  
Short Note ◽  
Solar Neutrinos ◽  
Asymptotic Giant Branch ◽  
Close Binaries ◽  
Asymptotic Giant Branch Stars ◽  
Radio Pulsars ◽  
Recent Developments ◽  
Late Evolution ◽  
Giant Branch Stars ◽  
Millisecond Radio

In previous reports, short reviews of the recent developments in a few selected major topics have revealed themselves very valuable and we go on with this useful practise. The subjects are: Stars of very low luminosity: red, brown and white dwarfs (F. D’Antona), Solar models (P. Demarque) and a short note on The observation of the solar neutrinos by the Kamiokande collaboration (Y. Totsuka), The HR diagrams for massive stars in the Magellanic Clouds (Ed. L. Fitzpatrick), Late evolution of asymptotic giant branch stars: clues from IR and radio observations (S. Kwok), SN 1987A (J.C. Wheeler), Binary and millisecond radio pulsars and evolution of close binaries (E. van den Heuvel), Progresses in computational methods for stellar models (G. Meynet). I am very grateful to the authors for providing promptly these very useful reviews.

Helium and Carbon‐Oxygen White Dwarfs in Close Binaries

1997 ◽  
Vol 475 (1) ◽  
pp. 291-299 ◽  
Author(s):  
Icko Iben, Jr. ◽  
Alexander V. Tutukov ◽  
Lev R. Yungelson
Keyword(s):  
White Dwarfs ◽  
Close Binaries

scholarly journals Massive close binaries and evolutionary synthesis of young starbursts

1999 ◽  
Vol 193 ◽  
pp. 596-597
Author(s):  
Dany Dionne
Keyword(s):  
Magellanic Clouds ◽  
Evolutionary Synthesis ◽  
Close Binaries

With an evolutionary synthesis code, I follow the evolution of a starburst composed of massive close binaries (MCBs) and of single stars at various metallicities. Evolutionary tracks for MCBs have been developed in collaboration with D. Vanbeveren and C. de Loore. The models reproduce the observed WR/O ratio in the Magellanic Clouds.

scholarly journals Tidal Circularization Among the Close Binaries in M67

1992 ◽  
Vol 151 ◽  
pp. 471-472
Author(s):  
David W. Latham ◽  
Robert D. Mathieu ◽  
Alejandra A. E. Milone ◽  
Robert J. Davis
Keyword(s):  
Main Sequence ◽  
Open Cluster ◽  
Radial Velocities ◽  
Spectroscopic Binaries ◽  
Close Binaries ◽  
To Come ◽  
Mirror Telescope

In 1971 Roger Griffin and Jim Gunn began monitoring the radial velocities of most of the members brighter than the main-sequence turnoff in the old open cluster M67, primarily using the 200-inch Hale Telescope. In 1982 the torch was passed to Dave Latham and Bob Mathieu, who began monitoring many of the same stars with the 1.5-meter Tillinghast Reflector and the Multiple-Mirror Telescope on Mt. Hopkins. We have successively combined these two sets of data, plus some additional CORAVEL velocities kindly provided by Michel Mayor, to obtain 20 years of time coverage (e.g. Mathieu et al. 1986). Among the stars brighter than magnitude V = 12.7 we have already published orbits for 22 spectroscopic binaries (Mathieu et al. 1990). At Mt. Hopkins an extension of this survey to many of the cluster members down to magnitude V = 15.5 has already yielded thirteen additional orbital solutions, with the promise of many more to come.

scholarly journals Inverse tides in pulsating binary stars

2020 ◽  
Vol 501 (1) ◽  
pp. 483-490
Author(s):  
Jim Fuller
Keyword(s):  
Binary Stars ◽  
Close Binary ◽  
Close Binaries ◽  
Spin Orbit ◽  
Misalignment Angle ◽  
Stellar Rotation ◽  
Transfer Energy ◽  
Pulsating Stars ◽  
Mode Amplitude ◽  
Rotation Periods

ABSTRACT In close binary stars, the tidal excitation of pulsations typically dissipates energy, causing the system to evolve towards a circular orbit with aligned and synchronized stellar spins. However, for stars with self-excited pulsations, we demonstrate that tidal interaction with unstable pulsation modes can transfer energy in the opposite direction, forcing the spins of the stars away from synchronicity, and potentially pumping the eccentricity and spin–orbit misalignment angle. This ‘inverse’ tidal process only occurs when the tidally forced mode amplitude is comparable to the mode’s saturation amplitude, and it is thus most likely to occur in main-sequence gravity mode pulsators with orbital periods of a few days. We examine the long-term evolution of inverse tidal action, finding the stellar rotation rate can potentially be driven to a very large or very small value, while maintaining a large spin–orbit misalignment angle. Several recent asteroseismic analyses of pulsating stars in close binaries have revealed extremely slow core rotation periods, which we attribute to the action of inverse tides.

scholarly journals Search for dormant black holes in ellipsoidal variables III. The OGLE BULGE short-period sample

2021 ◽  
Author(s):  
Roy Gomel ◽  
Simchon Faigler ◽  
Tsevi Mazeh ◽  
Michał Pawlak
Keyword(s):  
Main Sequence ◽  
Compact Object ◽  
Close Binaries ◽  
Periodic Modulation ◽  
Mass Ratio ◽  
True Nature ◽  
The Third ◽  
Short Period ◽  
Actual Mass

Abstract This is the third of a series of papers that presents an algorithm to search for close binaries with massive, possibly compact, unseen secondaries. The detection of such a binary is based on identifying a star that displays a large ellipsoidal periodic modulation, induced by tidal interaction with its companion. In the second paper of the series we presented a simple approach to derive a robust modified minimum mass ratio (mMMR), based on the observed ellipsoidal amplitude, without knowing the primary mass and radius, assuming the primary fills its Roche lobe. The newly defined mMMR is always smaller than the actual mass ratio. Therefore, a binary with an mMMR larger than unity is a good candidate for having a massive secondary, which might be a black hole or a neutron star. This paper considers 10,956 OGLE short-period ellipsoidals observed towards the Galactic Bulge. We re-analyse their modulation and identify 136 main-sequence systems with mMMR significantly larger than unity as candidates for having compact-object secondaries, assuming their observed periodic modulations reflect indeed the ellipsoidal effect. Obviously, one needs follow-up observations to find out the true nature of these companions.

Intrinsic Variables as Components of Close Binaries

2005 ◽  
Vol 296 (1-4) ◽  
pp. 145-155 ◽  
Author(s):  
N. N. Samus
Keyword(s):  
Close Binaries
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