2005IAUC.8523....4R


Query : 2005IAUC.8523....4R

2005IAUC.8523....4R - IAU Circ., 8523, 4 (2005/May-0)

V5115 Sagittarii.

RUDY R.J., RUSSELL R.W. and LYNCH D.K.

Abstract (from CDS):

R. J. Rudy, R. W. Russell, and D. K. Lynch, Aerospace Corporation, report on 0.8-5.0-micron spectroscopy of this nova (cf. IAUC 8500, 8501) obtained on Apr. 17 with the Infrared Telescope Facility (+ SpeX). In addition to the emission features of hydrogen, V5115 Sgr showed the strong, fluorescently excited lines of O I that are typical of a nova shortly after outburst, along with many lines of N I, but no prominent features from C I. Widths (FWHM) for the stronger emission were 3000 km/s. Fe II emission was present but there was no evidence of the CO bands at 2.3 and 4.6 microns or thermal emission from dust. The reddening derived from the O I lines was E(B-V) = 0.53.

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.8523....4R

Basic data :
V* V5115 Sgr -- Classical Nova
Other object types:
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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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V* V5115 Sgr

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