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- W1994310609 abstract "We have observed the old nova NQ Vul (1976) in the |$J=2rightarrow 1$| rotational transition of 12CO. We see a broad, low-intensity feature centred at velocity 26 km s–1 relative to the local standard of rest, FWHM |$sim80,text{km s}^{-1}$| and peak antenna temperature 63 mK. The central VLSR is consistent with the distance ( 1.2 ± 0.5 kpc) and galactic coordinates of NQ Vul and we conclude that the CO is associated with the NQ Vul system. We discuss possible origins of this material and suggest that it represents material ejected by the NQ Vul system prior to its 1976 outburst." @default.
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- W1994310609 date "1989-09-01" @default.
- W1994310609 modified "2023-10-14" @default.
- W1994310609 title "Millimetre CO observation of the old nova NQ Vul" @default.
- W1994310609 doi "https://doi.org/10.1093/mnras/240.1.47p" @default.
- W1994310609 hasPublicationYear "1989" @default.
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