1983•Publications of the Astronomical Society of JapanRequires access

Possible detection of violet-shifted absorption and emission lines from HBV 475.

Shinichi Tamura

Abstract

On a obtenu des spectres de haute dispersion de HBV 475. Dans le spectre de novembre 1981, on a detecte trois raies d'absorption Fe I et trois raies d'emission [Fe II]. Ces raies sont decalees d'environ 10 A vers le violet. En novembre 1982, ces raies ont disparu. L'aspect de ces raies suggere un phenomene explosif dans la chromosphere heterogene de cet objet

About this research paper

What this paper is about

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.

Available abstract

Key concepts: Physics, Astrophysics, Emission spectrum, Absorption (acoustics), Optics, Spectral line, Astronomy