نتایج جستجو برای: binary star

تعداد نتایج: 186576  

2016
B. P. ABBOTT R. ABBOTT T. D. ABBOTT M. R. ABERNATHY F. ACERNESE K. ACKLEY C. ADAMS T. ADAMS P. ADDESSO R. X. ADHIKARI V. B. ADYA C. AFFELDT M. AGATHOS K. AGATSUMA N. AGGARWAL O. D. AGUIAR P. A. ALTIN S. B. ANDERSON W. G. ANDERSON K. ARAI M. C. ARAYA C. C. ARCENEAUX J. S. AREEDA J. C. BARAYOGA S. E. BARCLAY B. C. BARISH M. A. BIZOUARD J. K. BLACKBURN C. D. BLAIR D. G. BLAIR R. M. BLAIR P. R. BRADY V. B. BRAGINSKY A. F. BROOKS D. A. BROWN D. D. BROWN N. M. BROWN S. BRUNETT C. C. BUCHANAN H. Y. CHEN Y. CHEN C. CHENG A. CHINCARINI A. CHIUMMO H. S. CHO E. E. COWAN D. M. COWARD M. J. COWART D. C. COYNE

We report here the non-detection of gravitational waves from the merger of binary neutron star systems and neutron-star–black-hole systems during the first observing run of Advanced LIGO. In particular we searched for gravitational wave signals from binary neutron star systems with component masses ∈ [1,3]M and component dimensionless spins < 0.05. We also searched for neutron-star–black-hole s...

1998
Y. Eriguchi

In this paper we have examined numerically exact configurations of close binary systems composed of incompressible fluids with internal flows. Component stars of binary systems are assumed to be circularly orbiting each other but rotating nonsynchronously with the orbital motion, i.e. stars in binary systems have steady motions seen from a rotational frame of reference. We have computed several...

Journal: :Symposium - International Astronomical Union 2001

Journal: :Symposium - International Astronomical Union 1988

2000
Pavel Kroupa

The stellar-dynamical evolution of bound star clusters during the first few Myr is dominated by binary-binary and binary-star interactions, the rapid sinking of the most massive stars to the centre of the clusters and mass loss from evolving stars. The consequences of these processes for the binary and stellar population in clusters, and for the star clusters as a whole, are studied by followin...

Journal: :International Astronomical Union Colloquium 1984

2004
J. M. Fregeau P. Cheung F. A. Rasio

Physical collisions between stars occur frequently in dense star clusters, either via close encounters between two single stars, or during strong dynamical interactions involving binary stars. Here we study stellar collisions that occur during binary–single and binary–binary interactions, by performing numerical scattering experiments. Our results include cross sections, branching ratios, and s...

Journal: :Monthly Notices of the Royal Astronomical Society 1897

Journal: :International Astronomical Union Colloquium 1992

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