Results 121 to 130 of about 1,202 (206)

Can Isotopologues Be Used as Biosignature Gases in Exoplanet Atmospheres? [PDF]

Life (Basel), 2023
Glidden A, Seager S, Petkowski JJ, Ono S.   +3 more
europepmc   +1 more source

Mass-loss rates and dust-to-gas ratios for obscured Asymptotic Giant Branch stars of different metallicities

, 1999
J. Th. van Loon
openalex   +2 more sources

History of two mass loss processes in VY CMa. [PDF]

Proc Int Astron Union, 2023
Quintana-Lacaci G, Velilla L, Fonfría JP, Cernicharo J, Castro-Carrizo A, Agúndez M, Decin L.   +6 more
europepmc   +1 more source

Deep dredge-up in intermediate-mass thermally pulsing asymptotic giant branch stars [PDF]

, 2004
Richard J. Stancliffe, Christopher A. Tout, Onno R. Pols   +2 more
openalex   +1 more source

Reaction Rate Uncertainties and the Production of¹⁹F in Asymptotic Giant Branch Stars [PDF]

, 2004
Maria Lugaro, C. Ugalde, Amanda I. Karakas, J. Görres, M. Wiescher, John C. Lattanzio, Robert C. Cannon   +6 more
openalex   +1 more source

Carbonaceous dust grains seen in the first billion years of cosmic time. [PDF]

Nature, 2023
Witstok J, Shivaei I, Smit R, Maiolino R, Carniani S, Curtis-Lake E, Ferruit P, Arribas S, Bunker AJ, Cameron AJ, Charlot S, Chevallard J, Curti M, de Graaff A, D'Eugenio F, Giardino G, Looser TJ, Rawle T, Rodríguez Del Pino B, Willott C, Alberts S, Baker WM, Boyett K, Egami E, Eisenstein DJ, Endsley R, Hainline KN, Ji Z, Johnson BD, Kumari N, Lyu J, Nelson E, Perna M, Rieke M, Robertson BE, Sandles L, Saxena A, Scholtz J, Sun F, Tacchella S, Williams CC, Willmer CNA.   +41 more
europepmc   +1 more source

Modelling self-pollution of globular clusters from asymptotic giant branch stars [PDF]

, 2004
Yeshe Fenner, S. W. Campbell, Amanda I. Karakas, John C. Lattanzio, B. K. Gibson   +4 more
openalex   +1 more source

A New Approach to Identifying Red Supergiant Stars in Metal-poor Galaxies: A Case Study of NGC 6822

The Astrophysical Journal
A complete sample of red supergiant (RSG) stars is important for studying their properties. Identifying RSGs in extragalactic fields first requires removing the Galactic foreground dwarfs.
Zhi-wen Li, Ming Yang, Biwei Jiang, Yi Ren   +3 more
doaj   +1 more source

Common envelope binary interaction simulations between a thermally pulsating AGB star and a low mass companion. [PDF]

Mon Not R Astron Soc, 2022
González-Bolívar M, De Marco O, Lau MYM, Hirai R, Price DJ.   +4 more
europepmc   +1 more source

Eccentric Orbits of close Companions to Asymptotic Giant Branch Stars

, 2000
Noam Soker
openalex   +2 more sources