The Behavior of HgMn Stars in the Far-UV-Paper 7: HR 6000
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.
- Publication:
-
Research Notes of the American Astronomical Society
- Pub Date:
- June 2022
- DOI:
- Bibcode:
- 2022RNAAS...6..132M
- Keywords:
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- Chemically peculiar stars;
- 226
