New Direct Observational Evidence for Kicks in SNe

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dc.creatorTauris, T. M.
dc.creatorHeuvel, E. P. J. van den
dc.date2000-01-03
dc.date.accessioned2026-07-07T01:51:28Z
dc.date.available2026-07-07T01:51:28Z
dc.descriptionWe present an updated list of direct strong evidence in favour of kicks being imparted to newborn neutron stars. In particular we discuss the new cases of evidence resulting from recent observations of the X-ray binary Circinus X-1 and the newly discovered binary radio pulsar PSR J1141-6545. We conclude that the assumption that neutron stars receive a kick velocity at their formation is unavoidable (van den Heuvel & van Paradijs 1997).
dc.description2 pages, to appear in the proceedings of the IAU Colloq. 177 "Pulsar Astronomy - 2000 and beyond"
dc.identifierhttps://arxiv.org/abs/astro-ph/0001015
dc.identifierhttp://arxiv.org/abs/astro-ph/0001015
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/309
dc.subjectAstrophysics
dc.titleNew Direct Observational Evidence for Kicks in SNe
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