SIMBAD references

2014MNRAS.438.3483H - Mon. Not. R. Astron. Soc., 438, 3483-3489 (2014/March-2)

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

HOLDSWORTH D.L., RUSHTON M.T., BEWSHER D., WALTER F.M., EYRES S.P.S., HOUNSELL R. and DARNLEY M.J.

Abstract (from CDS):

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.

Abstract Copyright: © 2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society (2014)

Journal keyword(s): space vehicles: instruments - techniques: photometric - techniques: spectroscopic - novae, cataclysmic variables

Simbad objects: 7

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2020.02.19-20:26:30

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