Abstract
view Abstract Citations (11) References (28) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Evolution of a 0.7 Msun Red Giant Harpaz, Amos ; Kovetz, Attay ; Shaviv, Giora Abstract The evolution of a 0.7-solar mass red giant is followed along the red giant branch, with mass loss included according to Reimers's formula. The red giant star completes its evolution by totally exhausting its envelope, without igniting the helium in the core. At this point, the core mass, which turns into a white dwarf, is 0.43 solar mass. The consequences of such an evolutionary path are discussed, together with the constraints that these results impose on the mass-loss rate during this evolutionary phase. Publication: The Astrophysical Journal Pub Date: December 1987 DOI: 10.1086/165815 Bibcode: 1987ApJ...323..154H Keywords: Red Giant Stars; Stellar Evolution; Stellar Mass Ejection; Stellar Models; Mass Distribution; Milky Way Galaxy; Planetary Nebulae; Stellar Cores; Stellar Envelopes; Astrophysics; STARS: EVOLUTION; STARS: INTERIORS; STARS: LATE-TYPE; STARS: MASS LOSS full text sources ADS | data products SIMBAD (2)
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
