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- W85711916 abstract "view Abstract Citations (630) References (17) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS On the origin of planetary nebulae. Kwok, S. ; Purton, C. R. ; Fitzgerald, P. M. Abstract The stellar wind from a red giant produces an extensive cool circumstellar nebula of appreciable mass. It is suggested that in some cases mass loss continues until the hot core of the star is exposed and that the stellar wind from the remnant star collides with the circumstellar nebula, producing a relatively dense shell of gas which increases in mass and radius at a constant rate. It is shown that such a shell, when ionized by radiation from the central star, has the characteristics of a planetary nebula. V1016 Cygni is used as an example of a star which has recently undergone the transition from a red giant to a young low-mass planetary nebula. Publication: The Astrophysical Journal Pub Date: February 1978 DOI: 10.1086/182621 Bibcode: 1978ApJ...219L.125K Keywords: Astronomical Models; Planetary Evolution; Planetary Nebulae; Red Giant Stars; Stellar Winds; Interstellar Matter; Ionizing Radiation; Stellar Mass Ejection; Stellar Models; Astrophysics; Planetary Nebulae:Origin; Red Giants:Stellar Winds full text sources ADS | data products SIMBAD (1)" @default.
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- W85711916 date "1978-02-01" @default.
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- W85711916 title "On the origin of planetary nebulae" @default.
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