2003IAUC.8191....1B

Query : 2003IAUC.8191....1B

2003IAUC.8191....1B - IAU Circ., 8191, 1 (2003/September-0)

Possible nova in Scutum.

BOECHE C. and MUNARI U.

Abstract (from CDS):

C. Boeche and U. Munari, Asiago Observatory, report on spectroscopy (range 372-491 nm; disperson 0.23 nm/pixel) of the possible nova reported on IAUC 8190, using the Asiago 1.22-m telescope on Aug. 31.97 UT under somewhat-cloudy conditions: "The Balmer series is weakly in emission down to H_epsilon, and the line width is not appreciably larger than the instrumental profile (300 km/s). The Balmer-line profiles show a weak absorption component blueshifted by 500 km/s and a second emission peak redshifted by 650 km/s with respect to the main emission line. The well-developed absorption spectrum closely match that of a normal F2 supergiant, with normal intensity for s-element lines of Ba II (455.4 nm) and Sr II (407.8, 421.6 nm). A definitive classification with classical novae must await future spectroscopic and photometric development."

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....1B

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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