ScholarLens Back to search
1989•NASA Technical Reports Server (NASA)Requires access

Long-term variability and possible stellar cycles in hybrid-chromosphere stars

Anthony Veale, Alexander Brown

Open publisher page 0 citations

Abstract

Results from an investigation of the variability seen in the Mg II emission line fluxes and wind absorption components of a number of hybrid-chromosphere stars are presented. One star shows evidence of stellar cycle activity with a period on the order of 2000 days.

About this research paper

What this paper is about

Results from an investigation of the variability seen in the Mg II emission line fluxes and wind absorption components of a number of hybrid-chromosphere stars are presented. One star shows evidence of stellar cycle activity with a period on the order of 2000 days.

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

Results from an investigation of the variability seen in the Mg II emission line fluxes and wind absorption components of a number of hybrid-chromosphere stars are presented. One star shows evidence of stellar cycle activity with a period on the order of 2000 days.

Key concepts: Chromosphere, Astrophysics, Stars, Physics, Astronomy, T Tauri star, K-type main-sequence star, Term (time)

Related papers

Related paper 1Related paper 2Related paper 3
Back to paper searchBrowse research topicsOriginal source
Long-term variability and possible stellar cycles in hybrid-chromosphere stars — Research Paper | ScholarLens