New Swift/XRT observation shows faint X-ray transient SAX J1806.5-2215 remains active 1 year after outburst

Authors
Publication date 2012
Journal The astronomer's telegram
Volume | Issue number 3926
Pages (from-to) 1
Organisations
  • Faculty of Science (FNWI) - Anton Pannekoek Institute for Astronomy (API)
Abstract The faint X-ray transient SAX J1806.5-2215 was discovered through the detection of two type-I bursts by BeppoSAX's WFC in 1996-1997 (in't Zand et al. 1999, NuPhS, 69, 228). Around the times of both bursts, no persistent emission was detected from the source with BeppoSAX. RXTE/ASM observations suggested that the source was active from early 1996 till late 1997 with an X-ray luminosity of ~ 1E+36 erg/s (for d=8 kpc; Cornelisse et al.
Document type Article
Language English
Published at http://www.astronomerstelegram.org/?read=3926
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