Abstract
AbstractA method of photoelectric photometry of the components of visual double stars is briefly described. Observations of ADS 9701 = δ Ser and of UV Aur = ADS 3934 B are presented to demonstrate the usefulness of this technique for the accurate photometry of variables in close visual double stars.
Sign-in/Register to access full text options 
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.
