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- W2029665393 abstract "Using CGS4 on UKIRT, we have obtained a 1.95–2.45 μm infrared (IR) spectrum of the primary candidate counterpart to the bright Z LMXB GX5-1.IR photometry by Naylor, Charles & Longmore and the astrometry of Jonker et al.had previously identified this star as the most likely counterpart to GX5-1.The spectrum presented here clearly shows Brackett γ and He lines in emission, for the first time confirming the identity of the counterpart.Similar to our previous spectroscopy of the Z source LMXBs Sco X-1 and Sco X-2 (Bandyopadhyay et al.1999), the K-band spectrum of GX5-1 shows emission lines only.We briefly discuss the implications of this spectrum for the nature of the Z sources." @default.
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- W2029665393 date "2003-04-11" @default.
- W2029665393 modified "2023-09-26" @default.
- W2029665393 title "Spectroscopic identification of the infrared counterpart to GX5-1" @default.
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- W2029665393 doi "https://doi.org/10.1046/j.1365-8711.2003.06519.x" @default.
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