From Miras to Planetary Nebulae: Which Path to Stellar Evolution? : Montpellier, France, September 4-7, 1989M. O. Mennessier, A. OMONT (Ed) Atlantica Séguier Frontières, 1990 - 565 pàgines |
Continguts
The evolution of red giants to white dwarfs a rewiew of the observational | 16 |
The space distribution of AGBstars invited paper | 42 |
Pulsation and evolution of Mira variables invited paper | 67 |
Pulsations of model Mira variables | 85 |
The environment of Miras from interferometry invited paper | 99 |
The behavior of absorption lines in the spectra of Mira variables | 113 |
Driving the wind of AGB stars by linear acoustic waves | 131 |
CO line ratios and mass loss rates of ZuchermanDyck survey stars | 158 |
IRAS observations of extended dust envelopes around evolved stars | 173 |
Towards a circumstellar silicate mineralogy invited paper | 186 |
Frases i termes més freqüents
abundance AGB stars assumed Astron Astrophys atmosphere binary bright C-rich calculations carbon stars central star circumstellar colour compared cool core density depends derived detected determined diagram discussed distance distribution dust effect emission energy envelope equation estimate et al evolution evolutionary expected Figure flux formation galactic given grains Habing halo higher important increase indicate infrared IRAS known Kwok larger limit lower luminosity maser mass loss rate mean measured method Miras objects observed obtained OH/IR stars optical outflow parameters period phase photometry planetary nebulae possible post-AGB present pressure properties pulsation radiation radius range ratio recent red giant References region relation sample sequence shell shock shown silicate similar sources spectra stellar stellar wind suggest Table temperature transition values variables variations velocity wind Wood