XTE and SAX observations of the Be/neutron star system RX J0146.9+6121

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dc.creatorMereghetti, S.
dc.creatorTiengo, A.
dc.creatorIsrael, G. L.
dc.creatorStella, L.
dc.date1999-12-08
dc.date.accessioned2026-07-07T02:34:51Z
dc.date.available2026-07-07T02:34:51Z
dc.descriptionWe report XTE and SAX observations of the X-ray pulsar RX J0146.9+612, the neutron star/Be binary system with the longest known spin period. Data obtained one month after the most recent outburst (July 1997), show that the source has returned to its normal luminosity of a few 10^34 erg/s while spin down continued at an average rate of about 5x10e-8 s/s.
dc.description6 pages, latex, 7 figures, Accepted for publication on Astronomy & Astrophysics
dc.identifierhttps://arxiv.org/abs/astro-ph/9912169
dc.identifierhttp://arxiv.org/abs/astro-ph/9912169
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/15411
dc.subjectAstrophysics
dc.titleXTE and SAX observations of the Be/neutron star system RX J0146.9+6121
dc.typetext

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