Volume 371, Number 2, May IV 2001
|Page(s)||638 - 642|
|Section||Interstellar and circumstellar matter|
|Published online||15 May 2001|
Armagh Observatory, College Hill, Armagh BT61 9DG, Northern Ireland e-mail: firstname.lastname@example.org; email@example.com
2 Department of Astronomy, University of Texas, Austin, TX 78712, USA e-mail: firstname.lastname@example.org
Corresponding author: V. M. Woolf, email@example.com
Accepted: 14 March 2001
We report a photometric and spectroscopic study of the hot extreme helium star LSS 5121. We found photometric variability, but no period was evident in its periodogram. This is consistent with the previous proposal, based on spectral line variations, that LSS 5121 is a non-radial pulsator similar to other hot extreme helium stars.
Key words: stars: chemically peculiar / stars: oscillations / stars: variables / stars: individual: LSS 5121
© ESO, 2001
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.