Monitoring of Mira (omi Cet) in support of HST Observations
Active Dates: Sept. 9, 2007 – Oct. 7, 2007
Abstract:
Dr. Margarita Karovska (Harvard-Smithsonian Center for Astrophysics) and collaborators are performing a comprehensive study of the Mira AB interacting system, using the WFPC2 camera on the Hubble Space Telescope.
Justification:
To determine the properties of the material ejected in December 2004 in the Mira AB system, its physical characteristics of mass transfer, and the system's response to the increased accretion rate onto Mira B.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| omi Cet | 2.00 | M |
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. Margarita Karovska; Imported Campaign (Alert Notice #358)