ScholarLens Back to search
1987•Trudy Astrofizicheskogo Instituta Alma-AtaRequires access

Radiative scattering in ion lines as the main cause of formation and heating of the stellar winds of hot stars.

Eh. Ya. Vil'Koviskij

Open publisher page 0 citations

Abstract

This record does not include an abstract. Use the full-text link above if available.

About this research paper

What this paper is about

An abstract is not available in the OpenAlex record for this paper.

Why it matters

A significance statement is not available in the OpenAlex record.

Key contribution

A contribution statement is not available in the OpenAlex record.

Method / approach

Method details are not available in the OpenAlex metadata.

Main findings

Findings are not separately available in the OpenAlex metadata.

Limitations

Limitations are not available in the OpenAlex metadata.

Applications

Application details are not available in the OpenAlex metadata.

Key concepts: Radiative transfer, Stars, Astrophysics, Physics, Scattering, Stellar atmosphere, Astronomy, Ion

Related papers

Related paper 1Related paper 2Related paper 3
Back to paper searchBrowse research topicsOriginal source
Radiative scattering in ion lines as the main cause of formation and heating of the stellar winds of hot stars. — Research Paper | ScholarLens