Volume 390, Number 1, July IV 2002
|Page(s)||109 - 119|
|Section||Galactic structure, stellar clusters, and populations|
|Published online||05 July 2002|
Rotation of stars in NGC 6134*
A comparison of δ Scuti stars and non-variable stars
Institute for Physics and Astronomy, University of Aarhus, Bygn. 520, 8000 Aarhus C, Denmark
2 Institut für Astronomie der Universität Wien, Türkenschanzstrasse 17, 1180 Wien, Austria
Corresponding author: S. Frandsen, email@example.com
Accepted: 24 April 2002
We present results of spectroscopic observations of selected stars in the southern open cluster NGC 6134. We have determined the rotational velocities of the six known δ Scuti stars in NGC 6134 as well as several other non-variable stars with similar colour temperature in order to investigate if and variability is somehow connected: we find no such correlation. We also compare the distribution of of δ Scuti stars and non-variable stars with four other well-studied open clusters to look for any systematic behaviour, but we find no conclusive evidence for and variability to be connected. We have also used the spectra to carry out an abundance analysis of the δ Scuti stars in NGC 6134 to confirm the high metal content of the cluster. We find which is in agreement with the result obtained from Strömgren photometry. We also present photometry of the cluster, but we find no chemical peculiar stars based on this index.
Key words: stars: oscillations / stars: variable: δ Scuti / stars: rotation / open clusters and associations: individual: NGC 6134, NGC 3680
© ESO, 2002
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.