0735-40 CGCS 1825 - NEW RED VARIABLE IN PUPPIS
Abstract:
Paul Camilleri, Cobram, Victoria, Australia, has discovered a new variable, likely a long period variable, in Puppis at magnitude 9.5 on three films taken January 7.508 UT using an 85-mm camera lens. Camilleri also observed the star visually on Jan 8.47 at magnitude 9.5 with a strong red color.
Justification:
Observers are encouraged to monitor this variable now, while it appears to be near maximum, and throughout its entire cycle, so that its nature may be determined. Because the star is so red, please be very careful in making your observations that you do not look at the variable for any length of time.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| USNO-B1.0 0735-0599207 | 17.00 | DQ+E |
Cadence: Not Specified Precision: 100 mmag |
Not Requested |
Spectroscopy Lines:
No spectroscopy lines provided
Photometry Filters:
B (Johnson), V (Johnson), r (Sloan), i (Sloan)
Comparison Stars:
Finder charts with comparison stars may be created using the AAVSO Variable Star Plotter (VSP).
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: Paul Camilleri; Imported Campaign (Alert Notice #269)