Anticipated primary eclipse of b Persei in January 2020
Abstract:
The bright (4.6 V) triple-star, eclipsing system b Persei has been the subject of several AAVSO campaigns. The current campaign requests high time-resolved observations of the bright star b Persei during the upcoming predicted primary eclipse, or transit, of the third star across the system.
Justification:
The recent campaigns by AAVSO observers have revealed significant light curve dips and Radial velocity observations indicate this event is another opportunity to gather critical data on the b Persei system.
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, Dr. Robert Zavala, Jason Sanborn, Dr. Anatoly Miroshnichenko; Imported Campaign (Alert Notice #688)