Alert Notice 800: Photometry needed for five YSO stars in support of spectroscopy

Active Dates: Nov. 17, 2022 – Nov. 30, 2022


Abstract:

Ruhee Kahar (University of Dundee) and colleagues at several institutions have requested AAVSO observers' assistance in monitoring five YSO stars in support of high-resolution spectra data obtained with CARMENES in a study of accreting young stars. The targets are given in the table below.

Justification:

We are taking repeated high-resolution spectra of intermediate-mass young stars to study the velocities and temporal variability of accretion related lines in these objects. The sample of stars includes HAeBe stars and massive T Tauri stars that will evolve into A and B stars. The connection between both types is at present unclear and may be related to the magnetic activity of the future star. Previous observations of these objects also indicate some evidence of extinction by circumstellar material.

Requested Data Types:

Photometry



Targets
Name Magnitude Variability Type Photometry Notes Spectroscopy Notes
RY Tau 9.30 CTTS/ROT

Cadence: Not Specified

Precision: 100

Not Requested
UX Ori 9.40 UXOR

Cadence: Not Specified

Precision: 100

Not Requested
RR Tau 10.20 UXOR

Cadence: Not Specified

Precision: 100

Not Requested
CO Ori 9.90 UXOR

Cadence: Not Specified

Precision: 100

Not Requested
R Mon 10.70 UXOR

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: Ruhee Kahar; Imported Campaign (Alert Notice #800)