2003IAUC.8191....2L

Query : 2003IAUC.8191....2L

2003IAUC.8191....2L - IAU Circ., 8191, 2 (2003/September-0)

Possible nova in Scutum.

LILLER W. and FUJII M.

Abstract (from CDS):

W. Liller, Vina del Mar, Chile, reports that an objective- prism spectrum taken on Aug. 31.093 UT shows a very narrow and weak H_alpha emission with a peak approximately 0.47 times the intensity of the nearby continuum; the FWHM appears to be no more than 300 km/s. M. Fujii, Kurashiki, Okayama, Japan, reports that a low- dispersion spectrum (range 390-850 nm; resolution about 1 nm), obtained on Aug. 31.55 UT with a 0.28-m reflector, shows emission lines of H_alpha (FWHM 700 km/s), H_beta, and Fe II (multiplets 42, 46, 49, 55, 74), with the Na I D absorption line.

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 EQ J184938-093345 No* 18 49 38 -09 33.7           ~ 3 0

Query : 2003IAUC.8191....2L

Basic data :
EQ J184938-093345 -- Classical Nova
Other object types: otypes_help 		No* ()
ICRS coord. (ep=J2000) : 		18 49 38.0 -09 33 42 [ ] E 2003IAUC.8190....1N
FK4 coord. (ep=B1950 eq=1950) : 		18 46 53.2 -09 37 12 [ ]
Gal coord. (ep=J2000) : 		024.2044 -03.9469 [ ]
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Identifiers (1) :
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EQ J184938-093345

References (3 between 1850 and 2026) (Total 3)
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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