867 citations
- Max Planck Institute for Gravitational PhysicsDE2 papers
- Scuola Internazionale Superiore di Studi AvanzatiIT2 papers
- Smithsonian Tropical Research InstitutePA2 papers
- University of California, RiversideUS2 papers
- University of EdinburghGB2 papers
- University of GeorgiaUS2 papers
- University of PaduaIT2 papers
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- Weizmann Institute of ScienceIL2 papers
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- Arcetri Astrophysical ObservatoryIT1 paper
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6 papers · 1 filter
High energy neutrinos from a slow jet model of core collapse supernovae
Soebur Razzaque, Peter Meszaros, Eli Waxman
It has been hypothesized recently that core collapse supernovae are triggered by mildly relativistic jets following observations of radio properties of these explosions. Associatio…
Enhancement of the flux from astrophysical sources by two photon annihilation interactions
Soebur Razzaque, Peter Meszaros, Eli Waxman
The ratio of anti-electron to total neutrino flux, , expected from interactions in astrophysical sources is . We point out that this ratio is enhance…
COUP census of X-ray stars in BN-KL and OMC-1S
N. Grosso, E. D. Feigelson, K. V. Getman +11
We present a study of the X-ray sources detected in the vicinity of two density peaks in the Orion Molecular Cloud 1 (OMC-1) behind the Orion Nebula Cluster (ONC), as seen in the e…
XMM-Newton observation of the drifting pulsar B0943+10
Bing Zhang, Divas Sanwal, George G. Pavlov
Radio pulsar subpulse drifting has been interpreted as rotation of sub-beams (sparks) of pair plasma produced by intermittent breakdowns of an inner vacuum gap above the pulsar pol…
Maximum elastic deformations of compact stars with exotic equations of state
Benjamin J. Owen
I make the first estimates of maximum elastic quadrupole deformations sustainable by alternatives to conventional neutron stars. Solid strange quark stars might sustain maximum ell…
Relativistic SPH Calculations of Compact Binary Mergers
Frederic Rasio, Joshua Faber, Shiho Kobayashi +1
We review recent progress in understanding the hydrodynamics of compact binary mergers using relativistic smoothed particle hydrodynamics (SPH) codes. Recent results are discussed…