SAX and XTE observations of GX 1+4, SMC X-1, RX J0146.9+6121 and 4U 0142+614, a sample of X-ray pulsators with extreme properties

Details SAX and XTE observations of GX 1+4, SMC X-1, RX J0146.9+6121 and 4U 0142+614, a sample of X-ray pulsators with extreme properties SAX and XTE observations of GX 1+4, SMC X-1, RX J0146.9+6121 and 4U 0142+614, a sample of X-ray pulsators with extreme properties

Jan 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999nuphs..69..141i&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 69, Issue 1-3, p. 141-144.

Physics

Nuclear Physics

1

Scientific paper

We report and discuss preliminary results obtained from the analysis of a sample of X-ray pulsars observed by SAX and XTE. The sample includes GX 1+4, a ~125s period low-mass X-ray pulsar which shows extreme properties and spin-up/down behaviour, 4U 0142+614, a member of the recently identified class of ``Anomalous'' X-ray pulsars, SMCX-1, a short period (~0.71s) X-ray pulsar in a high-mass binary, and RX J0146.9+6121, the slowest spinning accreting neutron star currently known (~25 min period).

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