2005IAUC.8501....3A

Query : 2005IAUC.8501....3A

2005IAUC.8501....3A - IAU Circ., 8501, 3 (2005/March-0)

Nova Sagittarii 2005.

AYANI K. and KAWABATA Y.

Abstract (from CDS):

K. Ayani and Y. Kawabata, Bisei Astronomical Observatory (BAO), report that their low-dispersion spectra (range 453-680 nm; resolution 0.6 nm at H_alpha) of this new object (IAUC 8500), obtained on Mar. 29.8 UT at the BAO 1.01-m telescope, also show it to be a nova, with H_alpha, H_beta, and Fe II (multiplet 42) lines having P-Cyg profiles. Preliminary analysis of the H_alpha emission (without decomposition of the absorption component) yields FWHM = 1300 km/s, the minimum of the H_alpha P-Cyg absorption being blueshifted by 1400 km/s with respect to the emission peak.

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* V5115 Sgr No* 18 16 59.04 -25 56 38.8           ~ 41 0

Query : 2005IAUC.8501....3A

Basic data :
V* V5115 Sgr -- Classical Nova
Other object types: otypes_help 		No* (2017ARep,NOVA), V* (V*)
ICRS coord. (ep=J2000) : 		18 16 59.04 -25 56 38.8 [ ] D 2005IAUC.8500....1N
FK4 coord. (ep=B1950 eq=1950) : 		18 13 52.81 -25 57 46.2 [ ]
Gal coord. (ep=J2000) : 		006.04636 -04.56739 [ ]
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Identifiers (4) :
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NOVA Sgr 2005 a NOVA Sgr 2005 V* V5115 Sgr p. NOVA Sgr 2005 No 1

References (41 between 1850 and 2026) (Total 41)
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* V5115 Sgr

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