2014MNRAS.438.3483H

Query : 2014MNRAS.438.3483H

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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Number of rows : 7
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 V* KT Eri No* 04 47 54.2014586736 -10 10 42.962267424   14.986 14.705 15.099   ~ 161 0
2 V* V382 Vel No* 10 44 48.3975221712 -52 25 31.168268472   15.945 15.737 16.173   ~ 201 0
3 V* RS Oph Sy* 17 50 13.1591484960 -06 42 28.480729788   11.884 10.776 11.228   K5.5/M0IIIe 1163 0
4 V* V5583 Sgr No* 18 07 07.67 -33 46 33.9           ~ 30 0
5 * alf Lyr dS* 18 36 56.33635 +38 47 01.2802 0.03 0.03 0.03 0.07 0.10 A0V 2787 1
6 V* V693 CrA No* 18 41 57.8 -37 31 14           ~ 125 0
7 V* V1370 Aql No* 19 23 21.2448589896 +02 29 26.326100040           ~ 172 0

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