Results 71 to 80 of about 983 (119)

Accelerated Free Energy Estimation in <i>Ab Initio</i> Path Integral Monte Carlo Simulations. [PDF]

open access: yesJ Phys Chem Lett
Svensson P   +6 more
europepmc   +1 more source

Completing the Spectral Mosaic of Chloromethane by Adding the CHD<sub>2</sub>Cl Missing Piece Through the Interplay of Rotational/Vibrational Spectroscopy and Quantum Chemical Calculations. [PDF]

open access: yesMolecules
Melosso M   +9 more
europepmc   +1 more source

Accurate geometric albedo, shape, and size of Hi'iaka from a stellar occultation. [PDF]

open access: yesNat Commun
Fernández-Valenzuela E   +73 more
europepmc   +1 more source

JWST Detects Silane in a Cold Low-Metallicity World

open access: yes
Faherty J   +30 more
europepmc   +1 more source

No exotic matter in asteroids. [PDF]

open access: yesEur Phys J Plus
Rubin AE, Burbine TH.
europepmc   +1 more source

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

open access: yes
Gilbert E   +35 more
europepmc   +1 more source

A time-independent, variational method for studying the photodissociation of triatomic molecules.

open access: yesPhys Chem Chem Phys
Pezzella M   +4 more
europepmc   +1 more source

Atmospheres of AGB Stars

2004
The use of the term atmosphere for the outer layers of a star is not obvious. The atmosphere of a terrestrial planet is easily defined as the gaseous envelope extending from the crust (or ocean) out into free space. For stars, the lower boundary is less easily defined.
Bengt Gustafsson, Susanne Höfner
openaire   +1 more source

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