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- W2005991520 abstract "view Abstract Citations (86) References (10) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Transition from a Red Giant to a Blue Nucleus after Ejection of a Planetary Nebula Harm, R. ; Schwarzschild, M. Abstract The evolution of two stars, with 0.65 M0 and 1.00 M0, respectively, has been computed through the transition phase following the rapid dynamical ejection of a planetary nebula by a red giant. This ejection phase was mimicked by a sequence of hydrostatic red-giant models with steadily decreasing mass. The sequence was terminated at the moment of rapid decrease of the previously high pulsational instability. With the starting model thus derived, the constant-mass transition phase was found to last about 6000 years. This time interval is just short enough that the star can start providing the ultraviolet radiation in time to excite the ejected nebula before the nebula completely disperses. Subject headings: interiors, stellar - late-type stars - planetary nebulae - stellar evolution Publication: The Astrophysical Journal Pub Date: September 1975 DOI: 10.1086/153790 Bibcode: 1975ApJ...200..324H full text sources ADS |" @default.
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- W2005991520 title "Transition from a Red Giant to a Blue Nucleus after Ejection of a Planetary Nebula" @default.
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