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STEREO/HI and optical observations of the classical nova V5583 Sagittarii

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Bewsher, Danielle ORCID: 0000-0002-6351-5170 (2014) STEREO/HI and optical observations of the classical nova V5583 Sagittarii. MNRAS, 438 (4). pp. 3483-3489.

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Other (STEREO/HI and optical observations of the classical nova V5583 Sagittarii)
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Official URL: https://doi.org/10.1093/mnras/stt2455

Abstract

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] &gsim; +1.0, which suggests that V5583 Sgr was most likely a neon nova.

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