Pulsating stars in NGC 6231: Frequency analysis and photometric mode identification near the main-sequence
Aims. We used Johnson UBV photometric CCD observations to identify pulsating and other variable stars in the young open cluster NGC 6231. The multi-colour information was used to classify pulsating variables, perform frequency analysis, and, where possibl
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|Source:||Astronomy and Astrophysics|
|01_Meingast_Pulsating_stars_in_NGC_6231:_2013.pdf||7.89 MB||Adobe PDF||Request a copy|
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