Monitoring of the Recurrent Nova U Scorpii
Active Dates: Jan. 22, 2008 – Jan. 22, 2010
Abstract:
Dr. Bradley E. Schaefer (Louisiana State University) requests increased monitoring of the recurrent nova U Scorpii (AAVSO 1616-17) over the next 24 months. Observers are asked to add U Sco to their regular observing program and to monitor the star in advance of an outburst predicted to occur around 2009.3 +/- 1.0 year.
Justification:
Schaefer predicts that because the nova outburst occurs after a certain amount of material collects on the white dwarf, and because the quiescent brightness of the star follows the mass accretion rate, we can predict when the accreted mass reaches the nova ignition point.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| U Sco | 7.50 | NR+E |
Cadence: Not Specified Precision: 100 |
Not Requested |
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. Bradley E. Schaefer; Imported Campaign (Alert Notice #367)