Volume 425 -
The Multifaceted Universe: Theory and Observations - 2022
(MUTO2022) -
Stars and interstellar medium
The Extremely He-rich Star HD144914
Full text:
pdf
Pre-published on:
September 30, 2022
Published on:
December 14, 2022
Abstract
HD144941 star is the most extreme representative of magnetic massive helium stars. In it, almost all atmospheric hydrogen is replaced by helium. Helium surface fraction 0.95 by quantity. Contents metals about 10 times less than solar in absolute number, the ratio of metals to hydrogen is typical of massive early-type stars.
DOI: https://doi.org/10.22323/1.425.0055
How to cite
Metadata are provided both in article format (very similar to INSPIRE) as this helps creating very compact bibliographies which can be beneficial to authors and readers, and in proceeding format which is more detailed and complete.
Open Access
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.
Copyright owned by the author(s) under the term of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License.