The Orbit of the High-Mass X-Ray Binary Pulsar 1E1145.1-6141

Astronomy and Astrophysics – Astrophysics

Scientific paper

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10 pages, 4 figures, accepted for publication in ApJ

Scientific paper

10.1086/344300

Observations of the 297 s X-ray pulsar 1E1145.1-6141 with the Rossi X-Ray
Timing Explorer have revealed its 14.4 d eccentric orbit around its B
supergiant companion. The best-fit orbital elements are: P_orb = 14.365(2) d,
a_x sin i=99.4(18) light-s, e=0.20(3). No eclipses are detected, indicating
that the binary inclination is less than 55 deg.

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