Far-infrared emission from ring nebulae

Details Far-infrared emission from ring nebulae Far-infrared emission from ring nebulae

Jul 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ap%26ss.205..283s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 205, no. 2, p. 283-295.

Astronomy and Astrophysics

Astronomy

3

Infrared Astronomy Satellite, Interstellar Matter, Nebulae, Stellar Spectra, Wolf-Rayet Stars, Cosmic Dust, O Stars

Scientific paper

Ring nebulae are known to form around stars like the WR and Of stars. The dust in these nebulae is heated by the central star and, therefore, provides a positive clue to the origin of the nebulae, complementing optical techniques. A systematic search has been carried out to study the infrared emission from these nebulae based on IRAS data. The influence of the local interstellar material properties on the formation of nebular dust is studied.

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