scholarly article | Q13442814 |
P819 | ADS bibcode | 1999ApJ...527L..39J |
P818 | arXiv ID | astro-ph/9908290 |
P356 | DOI | 10.1086/312397 |
P8608 | Fatcat ID | release_7h2l7d3uczb25m6qegn57onpbm |
P953 | full work available at URL | https://iopscience.iop.org/article/10.1086/312397/pdf |
P698 | PubMed publication ID | 10566994 |
P5875 | ResearchGate publication ID | 12734224 |
P2093 | author name string | Eberl T | |
Fryer CL | |||
Janka H | |||
Ruffert M | |||
P433 | issue | 1 | |
P407 | language of work or name | English | Q1860 |
P921 | main subject | black hole | Q589 |
P304 | page(s) | 39–42 | |
P577 | publication date | 1999-12-01 | |
P1433 | published in | The Astrophysical Journal | Q598789 |
P1476 | title | Black Hole-Neutron Star Mergers as Central Engines of Gamma-Ray Bursts. | |
P478 | volume | 527 |
Q61677326 | A theory of gamma-ray bursts |
Q68341975 | Active-sterile neutrino conversion: consequences for the r-process and supernova neutrino detection |
Q68511395 | Baryonic pollution in gamma-ray bursts: The case of a magnetically driven wind emitted from a disk orbiting a stellar mass black hole |
Q37598863 | Binary Neutron Star Mergers |
Q61677316 | Broad and Shifted Iron‐Group Emission Lines in Gamma‐Ray Bursts as Tests of the Hypernova Scenario |
Q39120904 | Coalescence of Black Hole-Neutron Star Binaries |
Q57954553 | Dynamical evolution of black hole-neutron star binaries in general relativity: Simulations of tidal disruption |
Q57429151 | Impact of an improved neutrino energy estimate on outflows in neutron star merger simulations |
Q68512115 | Kerr black holes and time profiles of gamma ray bursts |
Q57433251 | Low mass binary neutron star mergers: Gravitational waves and neutrino emission |
Q56573219 | Nucleosynthesis in neutron-rich ejecta from quark-novae |
Q57954605 | Post-Newtonian SPH calculations of binary neutron star coalescence: Method and first results |
Q57954598 | Post-Newtonian smoothed particle hydrodynamics calculations of binary neutron star coalescence. II. Binary mass ratio, equation of state, and spin dependence |
Q56484232 | SPH Methods in the Modelling of Compact Objects |
Search more.