2008IAUC.8957....1R

Query : 2008IAUC.8957....1R

2008IAUC.8957....1R - IAU Circ., 8957, 1 (2008/July-0)

V2671 Ophiuchi.

RUDY R.J., LYNCH D.K., RUSSELL R.W., GILBERT A.M. and WOODWARD C.E.

Abstract (from CDS):

R. J. Rudy, D. K. Lynch, R. W. Russell, and A. M. Gilbert, The Aerospace Corporation; and C. E. Woodward, University of Minnesota, report 0.8- to 5.5-micron spectroscopy of V2671 Oph on June 14 UT, obtained as above. V2671 Oph (Nova Oph 2008 No. 2; cf. IAUC 8951) is an "Fe II"-type nova with comparatively narrow lines of FWHM = 1200 km/s. It is at a very low stage of excitation, showing exceptionally bright lines of neutral carbon and strong emissison from the Ca II infrared triplet. The O I lines are also strong and indicate a large interstellar reddening of E(B-V) = 2.0. Weak, first-overtone emission from carbon monoxide beginning at 2.29 microns is present. No emission from dust is yet evident in the spectrum, but the presence of molecular gas suggests that its formation is imminent.

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* V2671 Oph No* 17 33 29.67 -27 01 16.4           ~ 16 0

Query : 2008IAUC.8957....1R

Basic data :
V* V2671 Oph -- Classical Nova
Other object types: otypes_help 		No* (2017ARep,NOVA), V* (V*)
ICRS coord. (ep=J2000) : 		17 33 29.67 -27 01 16.4 [ ] D 2008IAUC.8950....1N
FK4 coord. (ep=B1950 eq=1950) : 		17 30 22.09 -26 59 13.9 [ ]
Gal coord. (ep=J2000) : 		000.19866 +03.28523 [ ]
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Identifiers (2) :
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NOVA Oph 2008 b V* V2671 Oph

References (16 between 1850 and 2026) (Total 16)
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* V2671 Oph

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