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• W1974923907 abstract "The classical nova V5583 Sgr (Nova Sagittarii 2009 No 3) has been observed during the rise phase and shortly after by NASA's STEREO/HI instruments, with later optical spectroscopy obtained with the R-C Spectrograph at CTIO, Chile. The time of peak in the STEREO passband has been constrained to within 4 hours, as a result of the high cadence data obtained by STEREO/HI. The optical spectra show the nova evolving from the permitted to the nebular phases. The neon abundance in the ejecta is [Ne/O] > +1:0, which suggests that V5583 Sgr was most likely a neon nova." @default.
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• W1974923907 date "2014-01-20" @default.
• W1974923907 modified "2023-09-23" @default.
• W1974923907 title "STEREO/HI and optical observations of the classical nova V5583 Sagittarii" @default.
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• W1974923907 doi "https://doi.org/10.1093/mnras/stt2455" @default.
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