The ultimate outcome of black hole-neutron star mergers
- 1 January 2005
- journal article
- Published by Oxford University Press (OUP) in Monthly Notices of the Royal Astronomical Society
- Vol. 356 (1) , 54-58
- https://doi.org/10.1111/j.1365-2966.2004.08423.x
Abstract
No abstract availableKeywords
All Related Versions
This publication has 21 references indexed in Scilit:
- A very energetic supernova associated with the γ-ray burst of 29 March 2003Nature, 2003
- Formation of an Evanescent Proto–Neutron Star Binary and the Origin of Pulsar KicksThe Astrophysical Journal, 2002
- Study of Gamma‐Ray Burst Binary ProgenitorsThe Astrophysical Journal, 2002
- Newtonian hydrodynamics of the coalescence of black holes with neutron stars - IV. Irrotational binaries with a soft equation of stateMonthly Notices of the Royal Astronomical Society, 2001
- Newtonian hydrodynamics of the coalescence of black holes with neutron stars — III. Irrotational binaries with a stiff equation of stateMonthly Notices of the Royal Astronomical Society, 2000
- Black Hole–Neutron Star Mergers as Central Engines of Gamma-Ray BurstsThe Astrophysical Journal, 1999
- Formation Rates of Black Hole Accretion Disk Gamma‐Ray BurstsThe Astrophysical Journal, 1999
- Simulations of Binary Coalescence of a Neutron Star and a Black HoleThe Astrophysical Journal, 1998
- Identification of two classes of gamma-ray burstsThe Astrophysical Journal, 1993
- Discovery of a pulsar in a binary systemThe Astrophysical Journal, 1975