The formation of the black hole in the X-ray binary system V404 Cyg

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The formation of the black hole in the X-ray binary system V404 Cyg

Using new and archival radio data, we have measured the proper motion of the black hole X-ray binary V404 Cyg to be 9.2 ± 0.3 mas yr-1. Combined with the systemic radial velocity from the literature, we derive the full three-dimensional heliocentric space velocity of the system, which we use to calc...

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Bibliographic Details
Main Authors:	Miller-Jones, James, Jonker, P., Nelemans, G., Portegies Zwart, S., Dhawan, V., Brisken, W., Gallo, E., Rupen, M.
Format:	Journal Article
Published:	Wiley-Blackwell Publishing Ltd. 2009
Subjects:	stars: kinematics astrometry stars: supernovae: general stars: individual: V404 Cyg radio continuum: stars X-rays: binaries
Online Access:	http://onlinelibrary.wiley.com/doi/10.1111/j.1365-2966.2009.14404.x/full http://hdl.handle.net/20.500.11937/3291

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