V347 Aur monitoring requested in support of XMM-Newton
Active Dates: July 19, 2023 – Nov. 1, 2023
Abstract:
Monitoring the Young Stellar Object V347 Aur in support of XMM-Newton observations scheduled for August and possibly October to study optical outbursts and X-ray emissions.
Justification:
V347 Aur is a young low-mass star transitioning between an evolved protostar and a classical T Tauri star. It exhibits quasi-periodic optical outbursts, which likely indicate rapid mass-infalls that may also produce X-ray outbursts from star-disk magnetic interaction. Observing these outbursts can provide valuable data for comparison with XMM-Newton observations.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| BMAM-V347 | 17.45 | HADS |
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: Drs. Michael Richmond and Nicolas Grosso; Imported Campaign (Alert Notice #830)