1999A&A...347..975P

Query : 1999A&A...347..975P

1999A&A...347..975P - Astronomy and Astrophysics, volume 347975-982 (1999/7-3)

The ISO spectrum of the planetary nebula NGC 6302. II. Nebular abundances.

POTTASCH S.R. and BEINTEMA D.A.

Abstract (from CDS):

The ISO spectrum of NGC 6302 is used, in conjunction with the visible and ultraviolet spectrum, to determine the nebular composition. In addition to being considerably more accurate than previous determinations, the abundances of many more elements (and ions) can be found. A discussion of the previous evolution of the central star, in the light of these abundances, is given. A discussion is also given of the composition of the dust.

Abstract Copyright: ∼

Journal keyword(s): stars: abundances - stars: evolution - ISM: planetary nebulae: individual: NGC 6302 - infrared: ISM: lines and bands

Simbad objects: 5

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Number of rows : 5
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 M 42 HII 05 35 16.8 -05 23 15           ~ 4411 0
2 NAME Ori A MoC 05 38 -07.1           ~ 3187 0
3 NAME zet Oph Cloud Cld 16 37 09 -10 34.0           ~ 114 0
4 NGC 6302 PN 17 13 44.5 -37 06 11           O-rich 821 2
5 NGC 7027 PN 21 07 01.571952 +42 14 10.47120   10.358 8.831 10.157   ~ 2541 1

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