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2000ApJ...536..891N - Astrophys. J., 536, 891-895 (2000/June-3)
SAX J1810.8-2609: a new hard X-ray bursting transient.
NATALUCCI L., BAZZANO A., COCCHI M., UBERTINI P., HEISE J., KUULKERS E., IN'T ZAND J.J.M. and SMITH M.J.S.
Abstract (from CDS):
The detection of the type I X-ray burst is a strong indication that the compact object is a neutron star in a low-mass X-ray binary system. Assuming standard burst parameters and attributing the photospheric radius expansion to near-Eddington luminosity, we estimate a distance of ∼5 kpc. The inferred 2-10 keV X-ray luminosity is ∼9x1035 ergs.s–1 at the time of the discovery.
Abstract Copyright: ∼
Journal keyword(s): Stars: Binaries: Close - Stars: Individual: Alphanumeric: SAX J1810.8-2609 - X-Rays: Bursts
Simbad objects: 4
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