Holdsworth, D L, Rushton, M T, Bewsher, Danielle, Walter, F M, Eyres, Stewart Paul shore, Hounsell, R and Darnley, M J (2014) STEREO/HI and optical observations of the classical nova V5583 Sagittarii. Monthly Notices of the Royal Astronomical Society, 438 (4). pp. 3483-3489. ISSN 0035-8711
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Official URL: http://doi.org/10.1093/mnras/stt2455
The classical nova V5583 Sgr (Nova Sagittarii 2009 No 3) has been observed during the rise phase and shortly after by NASA's Solar TErrestrial RElations Observatory/Heliospheric Imager (STEREO/HI) instruments, with later optical spectroscopy obtained with the R-C Spectrograph at Cerro Tololo Inter-American Observatory, Chile. The time of peak in the STEREO passband has been constrained to within 4 h, 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.
|Uncontrolled Keywords (separate with ;):||space vehicles: instrument; techniques: photometric; techniques: spectroscopic; novae; cataclysmic variables|
|Subjects:||Physical sciences > Astronomy|
|Schools:||Faculty of Science and Technology > School of Physical Sciences and Computing > Jeremiah Horrocks Institute|
|Deposited By:||Nuala Jones|
|Deposited On:||09 Sep 2014 15:02|
|Last Modified:||18 Jan 2017 11:19|
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