Identification of the Periodic Hard X-Ray Transient GRO J1849-03 with the X-Ray Pulsar GS 1843-02 = X1845-024 - a New Be/X-Ray Binary

Details Identification of the Periodic Hard X-Ray Transient GRO J1849-03 with the X-Ray Pulsar GS 1843-02 = X1845-024 - a New Be/X-Ray Binary Identification of the Periodic Hard X-Ray Transient GRO J1849-03 with the X-Ray Pulsar GS 1843-02 = X1845-024 - a New Be/X-Ray Binary

1997-12-20

arxiv.org/abs/astro-ph/9712282v1

Astronomy and Astrophysics

Astrophysics

5 pages, 3 figures, accepted for publication in the Astrophysical Journal Letters

Scientific paper

10.1086/311189

We identify the periodic transient hard X-ray source GRO J1849-03 with the
transient x-ray pulsar GS 1843-02 = X1845-024 based on the detection of x-ray
outbursts from X1845-024 coincident with hard x-ray outbursts of GRO J1849--03.
Based on its spin period of 94.8 s and its orbital period of 241 days, we
classify the system as a Be/X-ray binary.

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