The ionization structure of planetary nebulae. IX. NGC 1535

Journal Article · Mon May 01 04:00:00 EDT 1989 · Astrophysical Journal; (USA)

DOI:https://doi.org/10.1086/167445· OSTI ID:5643952

Barker, T ^[1]

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1. Wheaton College, Norton, MA (USA)

The ionization structure of planetary nebula NGC 1535 was investigated using spectrophotometric observations of emission-line intensities over the spectral range 1400-7200 A, which were carried out in five positions in this nebula. The results obtained on the ionic abundances of He, O, N, Ne, C, and Ar in NGC 1535 suggest that it is a planetary nebula that formed initially in a somewhat metal-poor region and has undergone little or no enhancement of its original abundances by mixing with nuclear-processed material. 19 refs.

• OSTI ID: 5643952
• Journal Information: Astrophysical Journal; (USA), Journal Name: Astrophysical Journal; (USA) Vol. 340; ISSN ASJOA; ISSN 0004-637X
• Country of Publication: United States
• Language: English

Related Subjects

640102* -- Astrophysics & Cosmology-- Stars & Quasi-Stellar
Radio & X-Ray Sources
71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
ABUNDANCE
ARGON
ATTENUATION
BALMER LINES
CARBON
CHEMICAL COMPOSITION
ELEMENTS
EMISSION SPECTRA
FLUIDS
GASES
HELIUM
INTERSTELLAR SPACE
IONIZATION
MORPHOLOGY
NEBULAE
NEON
NITROGEN
NONMETALS
OXYGEN
PLANETARY NEBULAE
RARE GASES
SPACE
SPECTRA
SPECTROPHOTOMETRY
STAR EVOLUTION
ULTRAVIOLET SPECTRA