Results 181 to 190 of about 29,820 (298)

FORMATION OF SiC GRAINS IN PULSATION-ENHANCED DUST-DRIVEN WIND AROUND CARBON-RICH ASYMPTOTIC GIANT BRANCH STARS [PDF]

, 2012
Yuki Yasuda, Takashi Kozasa
openalex   +1 more source

Obscured Asymptotic Giant Branch stars in the Magellanic Clouds IV. Carbon stars and OH/IR stars [PDF]

, 1997
J. Th. van Loon, A. A. Zijlstra, P. A. Whitelock, P. te Lintel Hekkert, Jessica M. Chapman, C. Loup, M. A. T. Groenewegen, L. B. F. M. Waters, N. R. Trams   +8 more
openalex   +1 more source

Evidence of structural discontinuities in the inner core of red-giant stars. [PDF]

Nat Commun, 2022
Vrard M, Cunha MS, Bossini D, Avelino PP, Corsaro E, Mosser B.   +5 more
europepmc   +1 more source

The effect of thermally pulsating asymptotic giant branch stars on the evolution of the rest-frame near-infrared galaxy luminosity function [PDF]

, 2011
Bruno Henriques, Claudia Maraston, Pierluigi Monaco, Fabio Fontanot, Nicola Menci, Gabriella De Lucia, Chiara Tonini   +6 more
openalex   +1 more source

Synthesis of Organic and Inorganic Compounds in Asymptotic Giant Branch Stars

Galaxies
After the synthesis of carbon in the core of asymptotic giant branch (AGB) stars, carbon is dredged up to the surface by convection. Many carbon-based molecules are formed in the subsequently developed stellar wind.
Sun Kwok
doaj   +1 more source

Mixing and Magnetic Fields in Asymptotic Giant Branch Stars in the Framework of FRUITY Models [PDF]

, 2021
D. Vescovi
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Evolved Massive Stars at Low Metallicity. VII. The Lower Mass Limit of the Red Supergiant Population in the Large Magellanic Cloud

The Astrophysical Journal
The precise definition of the lower mass limit of red supergiant stars (RSGs) is an open question in astrophysics and does not attract much attention.
Ming Yang, Bo Zhang, Biwei Jiang, Jian Gao, Yi Ren, Shu Wang, Man I Lam, Hao Tian, Changqing Luo, Bingqiu Chen, Jing Wen   +10 more
doaj   +1 more source

Asymptotic Giant Branch Mass-loss Rates and Metal Yields from Scaled Mixing-length and Mass-loss Parameters

The Astrophysical Journal
Stars on the asymptotic giant branch (AGB) enrich the interstellar medium with carbon, nitrogen, and dust, which in turn boost cooling and promote future generations of planet and star formation.
Ezra Huscher, Kristian Finlator, Jason Jackiewicz   +2 more
doaj   +1 more source

Nucleosynthesis in asymptotic giant branch stars: Relevance for galactic enrichment and solar system formation

, 1999
M. Busso, R. Gallino, G. Wasserburg
semanticscholar   +1 more source

Probing clumpy pasts of galaxies from asymptotic giant branch stars [PDF]

, 2007
Kenji Bekki, Maria-Rosa L. Cioni
openalex   +1 more source