The Behavior of HgMn Stars in the Far-UV—Paper 7: HR 6000
Open Access
- 23 June 2022
- journal article
- Published by American Astronomical Society in Research Notes of the AAS
- Vol. 6 (6), 132
- https://doi.org/10.3847/2515-5172/ac7ab7
Abstract
The analysis of nine high resolution SWP spectra of the chemically peculiar star HR 6000 recorded by the International Ultraviolet Explorer reveals low amplitude variations of the far-ultraviolet flux (about 15% at 1500 Å) over the various observations with IUE. These variations could be caused by horizontal gradients of abundances of chemical elements over the surface of HR 6000.This publication has 3 references indexed in Scilit:
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- Catalogue of Ap, HgMn and Am starsAstronomy & Astrophysics, 2009
- A refined analysis of the remarkable Bp star HR 6000Astronomy & Astrophysics, 2007