2011CBET.2644....3I

Query : 2011CBET.2644....3I

2011CBET.2644....3I - Central Bureau Electronic Telegrams, 2644, 3 (2011/January-0)

Nova Sagittarii 2011 = PNV J17474639-2335112.

IMAMURA K.

Abstract (from CDS):

Kazuyoshi Imamura, Okayama University of Science (OUS), reports that a low-dispersion spectrum (R about 400) of PNV J17474639-2335112 was obtained on Jan. 28.886 UT with the 0.28-m Schmidt-Cassegrain telescope (+ DSS-7) at the OUS Observatory, showing a clear H_alpha emission line (FWHM approximately 1300 km/s), suggesting that the object is a classical nova. The spectrum is posted at http://blog-imgs-32-origin.fc2.com/t/n/b/tnblab/PN_Sgr_sp20110128.png.

Abstract Copyright: ∼

Journal keyword(s):

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* V5587 Sgr No* 17 47 46.33 -23 35 13.1           ~ 15 0

Query : 2011CBET.2644....3I

Basic data :
V* V5587 Sgr -- Classical Nova
Other object types: otypes_help 		No* (2017ARep,NOVA,...), V* (V*)
ICRS coord. (ep=J2000) : 		17 47 46.33 -23 35 13.1 [ ] D ~
FK4 coord. (ep=B1950 eq=1950) : 		17 44 43.44 -23 34 13.0 [ ]
Gal coord. (ep=J2000) : 		004.82488 +02.36226 [ ]
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Identifiers (4) :
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NOVA Sgr 2011 NOVA Sgr 2011 a PNV J17474639-2335112 V* V5587 Sgr

References (15 between 1850 and 2026) (Total 15)
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   

   

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V* V5587 Sgr

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