2012CBET.3072....2A

Query : 2012CBET.3072....2A

2012CBET.3072....2A - Central Bureau Electronic Telegrams, 3072, 2 (2012/March-0)

Nova Ophiuchi 2012 = PNV J17260708-2551454.

ARAI A. and ISOGAI M.

Abstract (from CDS):

Akira Arai and Mizuki Isogai, Koyama Astronomical Observatory (KAO), Kyoto Sangyo University, report that they obtained low-resolution (R about 550) spectrograms of PNV J17260708-2551454 with the 1.3-m Araki telescope at KAO on Mar. 27.74 UT. The spectra show prominent emission in H_alpha with P-Cyg profiles on a highly reddened continuum. H_beta, Fe II, and O I 777.4-nm are also visible. The FWHM of the H_alpha emission is about 600 km/s. These features suggest that the object is an "Fe II-type" classical nova. The spectra are posted at the following website URL: http://www.cc.kyoto-su.ac.jp/~kao/blog/index.php/view/165.

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* V2676 Oph No* 17 26 07.08 -25 51 45.4           ~ 43 0

Query : 2012CBET.3072....2A

Basic data :
V* V2676 Oph -- Classical Nova
Other object types: otypes_help 		No* (2017ARep,NOVA,...), V* (V*)
ICRS coord. (ep=J2000) : 		17 26 07.08 -25 51 45.4 [ ] D 2012CBET.3072....1N
FK4 coord. (ep=B1950 eq=1950) : 		17 23 01.32 -25 49 11.0 [ ]
Gal coord. (ep=J2000) : 		000.26315 +05.30129 [ ]
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Identifiers (4) :
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NOVA Oph 2012 NOVA Oph 2012 a PNV J17260708-2551454 V* V2676 Oph

References (43 between 1850 and 2026) (Total 43)
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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V* V2676 Oph

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