%0 Journal Article
%T The origin of the runaway high-mass X-ray binary HD153919/4U1700-37
%A A. Ankay
%A L. Kaper
%A J. H. J. de Bruijne
%A J. Dewi
%A R. Hoogerwerf
%A G. J. Savonije
%J Physics
%D 2001
%I arXiv
%R 10.1051/0004-6361:20010192
%X 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.
%U http://arxiv.org/abs/astro-ph/0102118v1