Evolution and merging of binaries with compact objects

[1]  Derek B. Fox,et al.  The Local Rate and the Progenitor Lifetimes of Short-Hard Gamma-Ray Bursts: Synthesis and Predictions for the Laser Interferometer Gravitational-Wave Observatory , 2006 .

[2]  G. E. Brown,et al.  Strangeness condensation by expanding about the fixed point of the Harada-Yamawaki vector manifestation. , 2005, Physical review letters.

[3]  G. Brown.  Hans Bethe 1906–2005 Hans Bethe's Nuclear Physics , 2005 .

[4]  D. Fox,et al.  The Local Rate and the Progenitor Lifetimes of Short-Hard Gamma-Ray Bursts: Synthesis and Predictions for LIGO , 2005, astro-ph/0511254.

[5]  J. Cordes,et al.  A 2.1 M☉ Pulsar Measured by Relativistic Orbital Decay , 2005, astro-ph/0508050.

[6]  I. Stairs,et al.  Binary radio pulsars , 2005 .

[7]  C. Santiapillai.  Hans Bethe (1906-2005) , 2005 .

[8]  J. Lattimer,et al.  The Physics of Neutron Stars , 2004, Science.

[9]  J. Dewi,et al.  The formation of the double neutron star pulsar J0737 − 3039 , 2003, astro-ph/0312152.

[10]  H. Bethe,et al.  Formation and evolution of black holes in the galaxy : selected papers with commentary , 2003 .

[11]  Chris L. Fryer,et al.  The Limiting Stellar Initial Mass for Black Hole Formation in Close Binary Systems , 2001, astro-ph/0112539.

[12]  Tomasz Bulik,et al.  A Comprehensive Study of Binary Compact Objects as Gravitational Wave Sources: Evolutionary Channels, Rates, and Physical Properties , 2001, astro-ph/0111452.

[13]  R.A.M.J. Wijers,et al.  Discovery of a Black Hole Mass-Period Correlation in Soft X-Ray Transients and Its Implication for Gamma-Ray Burst and Hypernova Mechanisms , 2001, astro-ph/0109538.

[14]  J. Telting,et al.  The mass of the neutron star in Vela X-1 , 2001, astro-ph/0108237.

[15]  T. Paradellis,et al.  12C(alpha,gamma)16O: the key reaction in stellar nucleosynthesis. , 2001, Physical review letters.

[16]  R. Wijers,et al.  The Evolution of Relativistic Binary Progenitor Systems , 2001, astro-ph/0103216.

[17]  S. Woosley,et al.  Presupernova Evolution with Improved Rates for Weak Interactions , 2000, astro-ph/0011507.

[18]  P. Madau,et al.  ApJ, in press Preprint typeset using L ATEX style emulateapj v. 04/03/99 ON THE ASSOCIATION OF GAMMA–RAY BURSTS WITH MASSIVE STARS: IMPLICATIONS FOR NUMBER COUNTS AND LENSING STATISTICS , 2000 .

[19]  D. Nice,et al.  On the Mass and Inclination of the PSR J2019+2425 Binary System , 2000, astro-ph/0010489.

[20]  J. Tauris.  On the energy equation and efficiency parameter of the common envelope evolution , 2000, astro-ph/0007034.

[21]  K. Langanke,et al.  Shell-model calculations of stellar weak interaction rates: II. Weak rates for nuclei in the mass range in supernovae environments , 2000, nucl-th/0001018.

[22]  V. Kaspi,et al.  Optical Observations of the Binary Pulsar System PSR B1718–19: Implications for Tidal Circularization , 1999, astro-ph/9908351.

[23]  T. Tauris,et al.  Formation of millisecond pulsars. I. Evolution of low-mass X-ray binaries with P_orb> 2 days , 1999, astro-ph/9909147.

[24]  N. Langer,et al.  Implications of massive close binaries for black hole formation and supernovae , 1999, astro-ph/9904256.

[25]  D. Chakrabarty,et al.  Neutron Star Mass Measurements. I. Radio Pulsars , 1998, astro-ph/9803260.

[26]  Hans A. Bethe,et al.  Evolution of Binary Compact Objects That Merge , 1998, astro-ph/9802084.

[27]  S. Zwart,et al.  Formation and evolution of binary neutron stars , 1997, astro-ph/9710347.

[28]  California Institute of Technology,et al.  The Pulsar kick velocity distribution , 1997, astro-ph/9708071.

[29]  Chris L. Fryer,et al.  Double Neutron Star Systems and Natal Neutron Star Kicks , 1997, astro-ph/9706031.

[30]  L. Cominsky,et al.  Observations of 4U 1700-37 with BATSE , 1996 .

[31]  Dong,et al.  pi N sigma term, s-bars in the nucleon, and the scalar form factor: A lattice study. , 1996, Physical review. D, Particles and fields.

[32]  J. Weingartner,et al.  On the formation of low-mass black holes in massive binary stars , 1995, astro-ph/9505092.

[33]  J. Cordes,et al.  A Millisecond Pulsar in a 6 Hour Orbit: PSR J0751+1807 , 1995 .

[34]  G. Brown.  Neutron star accretion and binary pulsar formation , 1995 .

[35]  H. Bethe,et al.  A Scenario for a Large Number of Low-Mass Black Holes in the Galaxy , 1994 .

[36]  V. Thorsson,et al.  Composition, structure and evolution of neutron stars with kaon condensates , 1993, nucl-th/9305006.

[37]  Daniel Schaerer,et al.  New grids of stellar models from 0.8 to 120 solar masses at Z = 0.020 and Z = 0.001 , 1992 .

[38]  S. Heap,et al.  Properties of the massive X-ray binary 4U 1700 - 37 = HD 153919 , 1992 .

[39]  D. Frail,et al.  An eclipsing millisecond pulsar in the globular cluster Terzan 5 , 1990, Nature.

[40]  A. Burrows,et al.  New Constraints on the Progenitor of the Binary Pulsar: PSR 1913+16 , 1986 .

[41]  R. Taam,et al.  Magnetic Field Decay and the Origin of Neutron Star Binaries , 1986 .

[42]  H. Bethe,et al.  Equation of state in the gravitational collapse of stars , 1979 .

[43]  P. Libby.  The Scientific American , 1881, Nature.

[44]  R. E. Casten,et al.  Nuclear Physics , 1935, Nature.

[45]  Physics Reports , 2022 .