Observations of the transient X-ray source 4U 0115+63

Details Observations of the transient X-ray source 4U 0115+63 Observations of the transient X-ray source 4U 0115+63

Aug 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979apj...231..919r&link_type=abstract

Astrophysical Journal, Part 1, vol. 231, Aug. 1, 1979, p. 919-926.

Astronomy and Astrophysics

Astrophysics

54

Binary Stars, Pulsars, Spectrum Analysis, X Ray Sources, X Ray Spectra, Ariel 5 Satellite, Energy Spectra, Heao 1, Light Curve, Satellite-Borne Instruments

Scientific paper

Results are presented for HEAO A-2 pointed observations and Ariel 5 A11-Sky Monitor observations of the X-ray transient 4U 0115 + 63. The transient source pulses with a period of 3.6136 s + or - 0.0004 s, has a hard spectrum typical of an X-ray binary pulsar, and has a broad iron line emission feature. A discussion of the transient behavior is given, and inferences are made concerning the nature of the X-ray source based on the pointed data.

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