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Astronomy and Astrophysics, ISSN 0004-6361, 10/2016, Volume 594, p. A97
.... One crucial ingredient in their modeling has been neglected: pair-instability pulsation supernovae with associated severe mass loss may suppress the formation... 
Gravitational waves | Black hole physics | Stars: massive | POPULATION | PROGENITORS | STAR-FORMATION | NEUTRON-STARS | EXPLOSION | METALLICITY | GRAVITATIONAL-WAVE DETECTION | RATES | black hole physics | STELLAR EVOLUTION | ASTRONOMY & ASTROPHYSICS | stars: massive | gravitational waves | M-CIRCLE-DOT | Physics - High Energy Astrophysical Phenomena
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2017, Volume 472, Issue 1, pp. 876 - 890
... and late-type main-sequence stars. By comparison of the obtained CME mass-loss rates with observations of total mass-loss rates, we find that our modelled rates may exceed those from observations by orders... 
Stars: mass-loss | Stars: late-type | Stars: activity | MAIN-SEQUENCE STARS | IN HABITABLE ZONES | TERRESTRIAL EXOPLANETS | DIFFERENTIAL ROTATION | CLASS FLARES | EARTH-LIKE EXOPLANETS | PROXIMA CENTAURI | stars: late-type | ASTRONOMY & ASTROPHYSICS | X-RAY-EMISSION | EXTREME-ULTRAVIOLET | stars: mass-loss | stars: activity | SOLAR-TYPE STARS | Physics - Solar and Stellar Astrophysics
Journal Article
Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 07/2015, Volume 453, Issue 1, pp. 357 - 364
... (inferred to be second generation stars in these models). If such mass-loss was due to tidal stripping, gas expulsion, or tidal interaction with the birth environment... 
Globular clusters: General | ABUNDANCE PATTERNS | globular clusters: general | HORIZONTAL-BRANCH | STAR-CLUSTERS | DYNAMICAL EVOLUTION | ASTRONOMY & ASTROPHYSICS | CHEMICAL-COMPOSITION | STELLAR POPULATIONS | LARGE-MAGELLANIC-CLOUD | GIANT STARS | MILKY-WAY | SELF-ENRICHMENT SCENARIOS | Physics - Astrophysics of Galaxies
Journal Article
Astronomy and Astrophysics, ISSN 0004-6361, 2010, Volume 509, Issue 1, p. A14
Context. Knowing how the mass loss of carbon-rich AGB stars depends on stellar parameters is crucial for stellar evolution modelling, as well as for the understanding of when and how circumstellar structures... 
Evolution - Stars | AGB and post-AGB - Stars | Mass-loss | Carbon - Circumstellar matter - Stars | Atmospheres - Stars | Stars | stars: atmospheres | MIRA VARIABLES | MECHANISM | stars: evolution | stars: AGB and post-AGB | stars: carbon | LONG-PERIOD VARIABLES | EVAPORATION | EVOLUTION | circumstellar matter | ASTRONOMY & ASTROPHYSICS | CHEMICAL-COMPOSITION | GROWTH | stars: mass-loss | RICH AGB-STARS | DETACHED SHELLS | ATMOSPHERIC DYNAMICS | Physics - Solar and Stellar Astrophysics
Journal Article