Campaign on Northern T Tau Stars

Active Dates: Nov. 12, 2020 – Dec. 17, 2020


Abstract:

Dr. Fred Walter (Stony Brook University) requests AAVSO observers to monitor 13 Northern T Tau stars in support of a multi-site multiwavelength campaign being carried out in November and December. The HST ULLYSES project is designed to obtain a statistically complete catalog of ultraviolet observations of a set of galactic stars while the HST can still obtain UV spectra. This AAVSO campaign will be part of a larger program called ODYSSEUS, which includes ground-based optical and near-IR photometry and spectroscopy.

Justification:

The goal of this observing campaign is to supplement the TESS photometry with filter photometry to distinguish the possible causes of brightenings and fadings in the light curve of T Tauri stars, including magnetic flares, enhanced accretion rates, starspots, and obscuration by a warped dust disk. The science goals are to understand the disk accretion processes that build up stars and drive their outbursts.

Requested Data Types:

Photometry



Targets
Name Magnitude Variability Type Photometry Notes Spectroscopy Notes
R Ori 9.05 M

Cadence: Not Specified

Precision: 100

Not Requested
TX Ori 11.70 CTTS

Cadence: Not Specified

Precision: 100

Not Requested
CVSO 11 15.57 WTTS

Cadence: Not Specified

Precision: 100

Not Requested
BMAM-V462 17.48 R

Cadence: Not Specified

Precision: 100

Not Requested
BMAM-V499 18.70 UG

Cadence: Not Specified

Precision: 100

Not Requested
NSV 2091 13.90 CTTS/ROT

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. Fred Walter; Imported Campaign (Alert Notice #725)