And Don't Forget The Black Holes

Simple item page
dc.creatorBethe, H. A.
dc.creatorBrown, G. E.
dc.creatorLee, C. -H.
dc.date2005-10-13
dc.date.accessioned2026-07-07T06:43:51Z
dc.date.available2026-07-07T06:43:51Z
dc.descriptionThe discovery of the highly relativistic neutron star (NS) binary (in which both NS's are pulsars) not only increases the estimated merging rate for the two NS's by a large factor, but also adds the missing link in the double helium star model of binary NS evolution. This model gives $\sim 20$ times more gravitational merging of low-mass black-hole (LMBH), NS binaries than binary NS's, whatever the rate for the latter is.
dc.description8pages, 1figure
dc.identifierhttps://arxiv.org/abs/astro-ph/0510378
dc.identifierhttp://arxiv.org/abs/astro-ph/0510378
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/102573
dc.subjectAstrophysics
dc.titleAnd Don't Forget The Black Holes
dc.typetext

Files

Collections

arXiv