Anticipated secondary eclipse of b Per centered on September 29 2022 UT
Active Dates: Sept. 19, 2022 – Oct. 8, 2022
Abstract:
Dr. Donald F. Collins, Dr. Robert Zavala, Jason Sanborn, and Dr. Anatoly Miroshnichenko have requested highly time-resolved observations of the bright star b Persei during the upcoming predicted secondary eclipse of the third star as it passes behind the AB inner pair.
Justification:
The close-orbiting binary pair shows ellipsoidal variation and the third star undergoes eclipses with the close-orbiting binary pair. Observations of these eclipses, both primary and secondary, contribute to understanding the system's dynamics.
Requested Data Types:
Photometry
Spectroscopy Lines:
No spectroscopy lines provided
Photometry Filters:
No photometry filters provided
Comparison Stars:
No comparison stars provided
Co-Authorship
Observers are not eligible for co-authorship.
Additional Observer Input:
Not provided
Additional Submission Location:
Not provided
Forum URL
N/A
Notes:
Principal Investigator: Dr. Donald F. Collins; Imported Campaign (Alert Notice #791)