IGR J19308+0530: Roche lobe overflow on to a compact object from a donor 1.8 times as massive

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IGR J19308+0530: Roche lobe overflow on to a compact object from a donor 1.8 times as massive

We present phase-resolved spectroscopy and photometry of the optical counterpart to the X-ray binary IGR J19308+0530. Ellipsoidal modulations in the light curve show that the F-type companion star in the system is Roche lobe filling. The optical spectra are dominated by absorption features from the...

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Bibliographic Details
Main Authors:	Ratti, E., van Grunsven, T., Torres, M., Jonker, P., Miller-Jones, James, Hessels, J., van Winkel, H., van der Sluys, M., Nelemans, G.
Format:	Journal Article
Published:	Wiley-Blackwell Publishing Ltd. 2013
Subjects:	novae stars: mass loss cataclysmic variables accretion: accretion discs X-rays: binaries stars: individual: IGR J19308+0530
Online Access:	http://hdl.handle.net/20.500.11937/5635

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