Abstract
Ground-based photometric observations are still the primary source of our knowledge of frequencies of modes excited in different types of pulsating stars. A typical set of photometric observations, accomplished usually by means of a multi-site campaign, allows to detect modes with amplitudes down to ∼0.1 mmag. The current abilities and limitations of this method of data collection are discussed in view of the requirements of the mode identification methods and asteroseismology. We also present some newest results of the multi-site campaign on stars in open cluster NGC6910.
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a callDisclaimer: All third-party content on this website/platform is and will remain the property of their respective owners and is provided on "as is" basis without any warranties, express or implied. Use of third-party content does not indicate any affiliation, sponsorship with or endorsement by them. Any references to third-party content is to identify the corresponding services and shall be considered fair use under The CopyrightLaw.
