XMM-Newton observing five T Tau stars
Abstract:
AAVSO observers are requested to monitor five T Tau stars to support XMM-Newton observations scheduled for the coming months. The study aims to analyze time variability in these stars over several weeks to months, which involves observing stars within the Taurus Molecular Cloud.
Justification:
It is crucial to study the interaction between stars, disks, and stellar flares during the early stages of star formation. Optical data before and after X-ray observations will help to correlate X-ray activity with optical lightcurve phases, potentially providing valuable insights into extinction events and other variabilities.
Requested Data Types:
Photometry
Targets
| Name | Magnitude | Variability Type | Photometry Notes | Spectroscopy Notes |
|---|---|---|---|---|
| tau 1 Ari | 5.26 | EB: |
Cadence: Not Specified Precision: 100 |
Not Requested |
| XZ Tau | 12.60 | CTTS/ROT |
Cadence: Not Specified Precision: 100 |
Not Requested |
| HL Tau | 14.30 | CTTS |
Cadence: Not Specified Precision: 100 |
Not Requested |
| BMAM-V710 | 16.00 | UG: |
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: Hans Moritz Guenther (MIT) and Christian Schneider (Universitaet Hamburg, Hamburger Sternwarte); Imported Campaign (Alert Notice #716)