Abstract
Initial findings are presented of wide integrated field photometry of several globular clusters, including the possibly highly relaxed cluster NGC 6864. The infrared data is compared with the visible integrated photometry data obtained by other authors to form intrinsic colours as a function of integrated field aperture, and is used to determine the infrared interstellar reddening.
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.
