The origin of the runaway high-mass X-ray binary HD153919/4U1700-37

Details The origin of the runaway high-mass X-ray binary HD153919/4U1700-37 The origin of the runaway high-mass X-ray binary HD153919/4U1700-37

2001-02-07

arxiv.org/abs/astro-ph/0102118v1

Astronomy and Astrophysics

Astrophysics

6 pages, latex, 3 embedded ps figures, to appear in A&A

Scientific paper

10.1051/0004-6361:20010192

Based on its Hipparcos proper motion, we propose that the high-mass X-ray binary HD153919/4U1700-37 originates in the OB association Sco OB1. At a distance of 1.9 kpc the space velocity of 4U1700-37 with respect to Sco OB1 is 75 km/s. This runaway velocity indicates that the progenitor of the compact X-ray source lost about 7 Msun during the (assumed symmetric) supernova explosion. The system's kinematical age is about 2 +/- 0.5 million years which marks the date of the supernova explosion forming the compact object. The present age of Sco OB1 is <8 Myr; its suggested core, NGC 6231, seems to be somewhat younger (~5 Myr). If HD153919/4U1700-37 was born as a member of Sco OB1, this implies that the initially most massive star in the system terminated its evolution within <6 million years, corresponding to an initial mass >30 Msun. With these parameters the evolution of the binary system can be constrained.

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