Results 321 to 330 of about 931,455 (366)

Precipitation induced by explosive volcanism on Mars and its implications for unexpected equatorial ice. [PDF]

Nat Commun
Hamid SS, Kerber L, Clarke AB.
europepmc   +1 more source

The punctuated evolution of the Venusian atmosphere from a transition in mantle convective style and volcanic outgassing. [PDF]

Sci Adv
Weller MB, Kiefer WS.
europepmc   +1 more source

Problems of stellar atmospheres.

The Astronomical Journal, 1948
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Planets larger than Neptune have elevated eccentricities. [PDF]

Proc Natl Acad Sci U S A
Gilbert GJ, Petigura EA, Entrican PM.
europepmc   +1 more source

Precise Masses Reveal that TOI-700 c is Low Density and TOI-700 d is Rocky

Gilbert E, Burt J, Barragán O, Siegel J, Mascareño AS, Silva A, Luque R, Rogers J, Lee E, Lopez E, Vanderburg A, Clement M, Youngblood A, Mamajek E, Sousa S, Cameron AC, Rodriguez J, Martin D, Arney G, Barclay T, Becker J, Colon K, Eisner N, Halverson S, Hord B, Kane S, Kreidberg L, Morley C, Mortier A, Nielsen L, Quintana E, Schlieder J, Suissa G, Triaud A, Trifonov T, Eylen VV.   +35 more
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A Tale of Sodium in Stellar and Planetary Atmospheres : Advancing transmission and million-star spectroscopy with 3D non-LTE radiative transfer

Canocchi, Gloria
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V3101 Cyg: A Cataclysmic Variable Born with a Brown Dwarf Donor

Ramirez S, Gänsicke B, Sahu S, Belloni D, Pala A, Koester D, Toloza O, Lagos-Vilches F.   +7 more
europepmc   +1 more source

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Stellar Atmosphere Modeling

2004
In this note, the formalism used to compute a simple stellar atmosphere model is described. The definition of a stellar atmosphere is strongly connected with the radiation field crossing the boundary layers of a star: the atmosphere is composed of those layers where photons interact with matter for the last time before leaving the star.
L. Chevallier
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Stellar Atmosphere Codes

Radiative Transfer in Stellar and Planetary Atmospheres, 2020
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