2009IAUC.9043....2P

Query : 2009IAUC.9043....2P

2009IAUC.9043....2P - IAU Circ., 9043, 2 (2009/May-0)

V1213 Centauri.

PIGULSKI A.

Abstract (from CDS):

A. Pigulski, Astronomical Institute, Wroclaw University, writes that he obtained a single spectrogram of the variable with the 1.9-m Radcliffe telescope (+ GIRAFFE echelle spectrograph; range 425-680 nm; resolution 32000) of the South African Astronomical Observatory on May 13.89 UT. The star shows very strong and broad emission in H-alpha, H-beta, and H-gamma. The peak flux of the H-alpha emission is roughly ten times stronger than that of the continuum. The FWHM of the Balmer lines (as measured from H-alpha and H-beta) corresponds to the velocity of 2300 km/s. In addition, the Fe II emission features at 490-540 nm, characteristic for a nova at an early stage of evolution, can be clearly seen in the spectrum.

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* V1213 Cen No* 13 31 15.8 -63 57 39           ~ 33 0

Query : 2009IAUC.9043....2P

Basic data :
V* V1213 Cen -- Classical Nova
Other object types: otypes_help 		No* (2017ARep,NOVA), V* (V*)
ICRS coord. (ep=J2000) : 		13 31 15.8 -63 57 39 (Optical) [ ] D 2003AstL...29..468S
FK4 coord. (ep=B1950 eq=1950) : 		13 27 50.2 -63 42 12 [ ]
Gal coord. (ep=J2000) : 		307.2862 -01.4263 [ ]
Fluxes (3) :
J 13.855 [0.01] B 2013A&A...554A.123S
H 13.664 [0.01] B 2013A&A...554A.123S
K 12.803 [0.01] B 2013A&A...554A.123S
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Identifiers (2) :
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NOVA Cen 2009 V* V1213 Cen

References (33 between 1850 and 2026) (Total 33)
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* V1213 Cen

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