Wang, Z. and Chakrabarty, D. and Roche, P. and Charles, P. A. and Kuulkers, E. and Shahbaz, T. and Simpson, C. and Forbes, D. A. and Helsdon, S. F. (2001) 'The optical counterpart of the accreting millisecond pulsar SAX J1808.4-3658 in outburst : constraints on the binary inclination.', Astrophysical journal : letters., 563 (1). L61-L64.
We present multiband optical/IR photometry of V4580 Sgr, the optical counterpart of the accretion-powered millisecond pulsar SAX J1808.4-3658, taken during the 1998 X-ray outburst of the system. The optical flux is consistent with emission from an X-rayheated accretion disk. Self-consistent modeling of the X-ray and optical emission during the outburst yields a best-fit extinction of AV=0.68+0.37-0.15 and an inclination of cosi=0.65+0.23-0.33 (90% confidence), assuming a distance of 2.5 kpc. This inclination range requires that the stellar companion of the pulsar has extremely low mass, Mc=0.050.10 M. Some of the IR observations are inconsistent with disk emission and are too bright to be from either the disk or the companion, even in the presence of X-ray heating.
|Keywords:||Accretion disks, Stars, Binaries, Pulsars, SAX J1808.4-3658, V4580 Sagittarii, Neutron.|
|Full text:||Full text not available from this repository.|
|Publisher Web site:||http://dx.doi.org/10.1086/338357|
|Record Created:||20 May 2008|
|Last Modified:||15 Mar 2011 12:36|
|Social bookmarking:||Export: EndNote, Zotero | BibTex|
|Usage statistics||Look up in GoogleScholar | Find in a UK Library|