2011IAUC.9203....2A

Query : 2011IAUC.9203....2A

2011IAUC.9203....2A - IAU Circ., 9203, 2 (2011/March-0)

V5588 Sagittarii = nova Sagittarii 2011 no. 2.

ARAI A., NAGASHIMA M., KAJIKAWA T. and NAKA C.

Abstract (from CDS):

A. Arai, M. Nagashima, T. Kajikawa, and C. Naka, Koyama Astronomical Observatory (KAO), Kyoto Sangyo University, report that low-resolution (R about 550) spectra of PNV J18102135-2305306 were obtained at the KAO on Mar. 28.725 UT under a hazy sky. The spectra show prominent emission lines of H_alpha, H_beta, and Fe II (multiplets 42, 48, 49) on a highly reddened continuum. The FWHM of the H_alpha emission line is about 900 km/s, and the Na D absorption line is also seen (equivalent width about 0.7 nm). These features suggest that the object is a classical nova that is reddened by interstellar matter.

Abstract Copyright: ∼

Journal keyword(s):

Status at CDS : Objects in title, abstract, text, figures, and all or part of small table(s) being processed in SIMBAD.

Simbad objects: 1

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Number of rows : 1
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* V5588 Sgr No* 18 10 21.3479238157 -23 05 30.044814019           ~ 39 0

Query : 2011IAUC.9203....2A

Basic data :
V* V5588 Sgr -- Classical Nova
Other object types: otypes_help 		No* (2017ARep,NOVA,...), CV* (2020MNRAS), V* (V*), * (Gaia)
ICRS coord. (ep=J2000) : 		18 10 21.3479238157 -23 05 30.044814019 (Optical) [ 0.5821 0.5280 90 ] A 2018yCat.1345....0G
FK4 coord. (ep=B1950 eq=1950) : 		18 07 19.1047090725 -23 06 08.333201142 [ 0.5821 0.5280 90 ]
Gal coord. (ep=J2000) : 		007.8399952193513 -01.8837006541989 [ 0.5821 0.5280 90 ]
Proper motions mas/yr : 		-4.062 -6.702 [1.203 1.043 90] A 2018yCat.1345....0G
Parallaxes (mas): 		1.1331 [0.6431] A 2018yCat.1345....0G
Fluxes (1) :
G 19.4228 [0.0267] C 2018yCat.1345....0G
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Identifiers (4) :
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NOVA Sgr 2011 b PNV J18102135-2305306 V* V5588 Sgr Gaia DR2 4066628490739652224

References (39 between 1850 and 2026) (Total 39)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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Distance : 1    Plx : 1    PM : 1   

   

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V* V5588 Sgr Gaia DR2 4066628490739652224

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