0735-40 CGCS 1825 - NEW RED VARIABLE IN PUPPIS

Active Dates: Jan. 7, 2000 – Jan. 14, 2000


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

Not Requested

Spectroscopy Lines:

No spectroscopy lines provided

Photometry Filters:

B (Johnson), V (Johnson), r (Sloan), i (Sloan)

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: Paul Camilleri; Imported Campaign (Alert Notice #269)