Results 341 to 350 of about 2,843,859 (384)

The erosion of large primary atmospheres typically leaves behind substantial secondary atmospheres on temperate rocky planets. [PDF]

Nat Commun
Krissansen-Totton J, Wogan N, Thompson M, Fortney JJ.   +3 more
europepmc   +1 more source

Laser-based approach to measure small nuclear cross sections in plasma. [PDF]

Proc Natl Acad Sci U S A
Feng J, Qi J, Zhang H, Chen S, Zhu M, Hu X, Xu H, Fu C, Wang X, Chen L, Zhang J.   +10 more
europepmc   +1 more source

Bogong moths use a stellar compass for long-distance navigation at night. [PDF]

Nature
Dreyer D, Adden A, Chen H, Frost B, Mouritsen H, Xu J, Green K, Whitehouse M, Chahl J, Wallace J, Hu G, Foster J, Heinze S, Warrant E.   +13 more
europepmc   +1 more source

The evolution of Gaia(s). [PDF]

Philos Trans R Soc Lond B Biol Sci
Lenton TM.
europepmc   +1 more source

The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant

Munoz-Sanchez G, Kalitsounaki M, de Wit S, Antoniadis K, Bonanos A, Zapartas E, Boutsia K, Christodoulou E, Maravelias G, Soszyński I, Udalski A.   +10 more
europepmc   +1 more source

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Stellar Evolution

Stars and Space with MATLAB Apps, 2020
Dozens of different types of stars populate the Milky Way Galaxy. The most common are main-sequence dwarfs like the Sun that fuse hydrogen into helium within their cores (the core of the Sun occupies about half its mass).
J. Kaler
semanticscholar   +2 more sources

The Luminosity function and stellar evolution

, 1955
The evolutionary significance of the observed luminosity function for main-sequence stars in the solar neighborhood is discussed. The hypothesis is made that stars move off the main sequence after burning about 10 per cent of their hydrogen mass and that
E. Salpeter
semanticscholar   +1 more source

Nucleosynthesis and Stellar Evolution

Astrophysics and Space Science, 2002
Two of the basic building blocks of galaxies are stars and the interstellar medium. The evolution of the abundance composition in the latter and especially the enrichment of heavy elements as a function of space and time reflects in turn the history of star formation and the lifetimes of the diverse contributing stellar objects.
Thielemann, F. K., Argast, D., Brachwitz, F., Martinez-Pinedo, G., Rauscher, T., Liebendorfer, M., Mezzacappa, A., Hoflich, P., Nomoto, K.   +8 more
openaire   +2 more sources

Fred’s Contributions to Stellar Evolution [PDF]

Astrophysics and Space Science, 2003
zbMATH Open Web Interface contents unavailable due to conflicting licenses.
openaire   +2 more sources