Discovery of a large and bright bow shock nebula associated with low-mass X-ray binary SAX J1712.6-3739

Type Journal Article
Names K. Wiersema, D. M. Russell, N. Degenaar, M. Klein-Wolt, R. Wijnands, S. Heinz, A. M. Read, R. D. Saxton, N. R. Tanvir
Publication Monthly Notices of the Royal Astronomical Society Letters
Volume 397
Issue 1
Pages L6-L10
Date July 1, 2009
Library Catalog NASA ADS
Abstract In a multiwavelength programme dedicated to identifying optical counterparts of faint persistent X-ray sources in the Galactic bulge, we find an accurate X-ray position of SAX J1712.6-3739 through Chandra observations, and discover its faint optical counterpart using our data from EFOSC2 on the ESO 3.6-m telescope. We find this source to be a highly extincted neutron star low-mass X-ray binary (LMXB) with blue optical colours. We serendipitously discover a relatively bright and large bow shock shaped nebula in our deep narrow-band Hα imaging, most likely associated with the X-ray binary. A nebula like this has never been observed before in association with a LMXB, and as such provides a unique laboratory to study the energetics of accretion and jets. We put forward different models to explain the possible ways the LMXB may form this nebulosity, and outline how they can be confirmed observationally.
Tags ISM: jets and outflows, X-Rays: Binaries
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