Abstract
The photometric activity of the star V695 Per in the young cluster IC 348 is studied using multi-year photometric observations. In terms of its photometric properties, this star is shown to be a twin of the well known T Tauri star AA Tau which is subject to periodic eclipses by its own gas-dust disk. It is suggested that, as in the case of AA Tau, the inner region of the circumstellar disk of V695 Per is deformed as a result of its interaction with a magnetic dipole whose axis is inclined to the star’s axis of rotation. This interpretation assumes that the line of sight lies nearly in the plane of the disk.
Full Text 
Sign-in/Register to access full text options
Sign-in/Register to access full text options 
Published version (
Free)
Free) 
Talk to us
Join us for a 30 min session where you can share your feedback and ask us any queries you have
Schedule a call
