2023Research Notes of the AASOpen access

The Behavior of He-weak in the Far-UV—Paper I: HD 5737

Richard Monier

Open full text 0 citations

Abstract

Abstract The analysis of 28 spectra of the bright B6 He-weak star HD 5737 recorded by the SWP camera on board the International Ultraviolet Explorer reveals one instance of marginal variation of the far-ultraviolet flux of this star from 1300 up to 1700 Å. All the other large aperture spectra show a remarkably constant spectral energy distribution. Over the 6 yr of the IUE mission, HD 5737 has experienced at least two episodes of very strong absorption in the C iv resonance lines at 1548.19 and 1550.77 Å,

About this research paper

What this paper is about

Abstract The analysis of 28 spectra of the bright B6 He-weak star HD 5737 recorded by the SWP camera on board the International Ultraviolet Explorer reveals one instance of marginal variation of the far-ultraviolet flux of this star from 1300 up to 1700 Å. All the other large aperture spectra show a remarkably constant spectral energy distribution. Over the 6 yr of the IUE mission, HD 5737 has experienced at least two episodes of very strong absorption in the C iv resonance lines at 1548.19 and 1550.77 Å,

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

Abstract The analysis of 28 spectra of the bright B6 He-weak star HD 5737 recorded by the SWP camera on board the International Ultraviolet Explorer reveals one instance of marginal variation of the far-ultraviolet flux of this star from 1300 up to 1700 Å. All the other large aperture spectra show a remarkably constant spectral energy distribution. Over the 6 yr of the IUE mission, HD 5737 has experienced at least two episodes of very strong absorption in the C iv resonance lines at 1548.19 and 1550.77 Å,

Key concepts: Far ultraviolet, Near ultraviolet, Ultraviolet, Spectral line, Astrophysics, Physics, Absorption spectroscopy, Resonance (particle physics)

Related papers

Back to paper searchBrowse research topicsOriginal source
The Behavior of He-weak in the Far-UV—Paper I: HD 5737 — Research Paper | ScholarLens