2005IAUC.8501....2K

Query : 2005IAUC.8501....2K

2005IAUC.8501....2K - IAU Circ., 8501, 2 (2005/March-0)

Nova Sagittarii 2005.

KISS L. and DEREKAS A.

Abstract (from CDS):

L. Kiss, University of Sydney; and A. Derekas, University of New South Wales, write that an optical spectrum (0.05 nm/pixel; range 580-675 nm), taken with the Australian National University 2.3-m telescope (+ Double-Beam Spectrograph) at Siding Spring Observatory on Mar. 29.81 UT, shows that the new object announced on IAUC 8500 is indeed a nova. The prominent H_alpha emission line shows a strong P-Cyg profile, with the main absorption component at -1300 km/s; there might also be a weak second component at -2100 km/s. The FWZI of the H_alpha line exceeds 5000 km/s. In addition to H_alpha, a few broad features are visible between 618 and 640 nm, also with P-Cyg-like profiles. The Na D doublet is saturated, indicating high interstellar reddening.

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....2K

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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