Search NASA⌕ Search

NASA NTRS · 19670021696

Models of stellar atmospheres

Abstract

Stellar atmosphere models that assume interior energy sources, thermodynamic and mechanical equilibrium, and absorption of radiant energy only in continuous spectrum

Explore related subjects

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Sobolev, V. V.. 1967-01-01. Models of stellar atmospheres. https://ntrs.nasa.gov/citations/19670021696

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related reports

An analysis of CH in the solar atmosphere.

CH molecule solar spectral observations interpreted using several upper photosphere models and assuming local thermodynamic equilibrium approximation

THERMODYNAMIC EQUILIBRIUM↗