Literature DB >> 16592476

Chemical composition of gaseous nebula NGC 6302.

L H Aller1, S J Czyzak.   

Abstract

The irregular emission nebula NGC 6302 exhibits a rich spectrum of lines ranging in excitation from [NI] to [FeVII]. An assessment of available spectroscopic data, covering a large intensity range, indicates excess of helium and nitrogen as compared with average planetary nebulae, but deficiencies in iron and calcium. These metals are presumably tied up in solid grains, as suggested by Shields for iron in NGC 7027.

Entities:  

Year:  1978        PMID: 16592476      PMCID: PMC411169          DOI: 10.1073/pnas.75.1.1

Source DB:  PubMed          Journal:  Proc Natl Acad Sci U S A        ISSN: 0027-8424            Impact factor:   11.205


  1 in total

1.  The chemical composition of the sun.

Authors:  J E Ross; L H Aller
Journal:  Science       Date:  1976-03-26       Impact factor: 47.728

  1 in total
  1 in total

1.  International Ultraviolet Explorer satellite observations of seven high-excitation planetary nebulae.

Authors:  L H Aller; C D Keyes
Journal:  Proc Natl Acad Sci U S A       Date:  1980-03       Impact factor: 11.205

  1 in total

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