OCCULTATION OF THE T TAURI STAR RW AURIGAE A BY ITS TIDALLY DISRUPTED DISK
Journal Article
·
· Astronomical Journal (New York, N.Y. Online)
- Department of Physics, Fisk University, 1000 17th Avenue North, Nashville, TN 37208 (United States)
- Department of Physics and Astronomy, Vanderbilt University, 6301 Stevenson Center, Nashville, TN 37235 (United States)
- Department of Astronomy, The Ohio State University, Columbus, OH 43210 (United States)
RW Aur A is a classical T Tauri star, believed to have undergone a reconfiguration of its circumstellar environment as a consequence of a recent flyby of its stellar companion, RW Aur B. This interaction stripped away part of the circumstellar disk of RW Aur A, leaving a tidally disrupted ''arm'' and a short truncated circumstellar disk. We present photometric observations of the RW Aur system from the Kilodegree Extremely Little Telescope survey showing a long and deep dimming that occurred from 2010 September until 2011 March. The dimming has a depth of ∼2 mag, a duration of ∼180 days, and was confirmed by archival observations from American Association of Variable Star Observers. We suggest that this event is the result of a portion of the tidally disrupted disk occulting RW Aur A, specifically a fragment of the tidally disrupted arm. The calculated transverse linear velocity of the occulter is in excellent agreement with the measured relative radial velocity of the tidally disrupted arm. Using simple kinematic and geometric arguments, we show that the occulter cannot be a feature of the RW Aur A circumstellar disk, and we consider and discount other hypotheses. We also place constraints on the thickness and semimajor axis of the portion of the arm that occulted the star.
- OSTI ID:
- 22273308
- Journal Information:
- Astronomical Journal (New York, N.Y. Online), Journal Name: Astronomical Journal (New York, N.Y. Online) Journal Issue: 5 Vol. 146; ISSN 1538-3881
- Country of Publication:
- United States
- Language:
- English
Similar Records
V409 Tau as another AA Tau: Photometric observations of stellar occultations by the circumstellar disk
Chandra resolves the T Tauri binary system RW Aur
DM ORI: A YOUNG STAR OCCULTED BY A DISTURBANCE IN ITS PROTOPLANETARY DISK
Journal Article
·
Wed Jul 01 00:00:00 EDT 2015
· The Astronomical Journal (Online)
·
OSTI ID:22879454
Chandra resolves the T Tauri binary system RW Aur
Journal Article
·
Fri Jun 20 00:00:00 EDT 2014
· Astrophysical Journal
·
OSTI ID:22356620
DM ORI: A YOUNG STAR OCCULTED BY A DISTURBANCE IN ITS PROTOPLANETARY DISK
Journal Article
·
Tue Nov 01 00:00:00 EDT 2016
· Astrophysical Journal
·
OSTI ID:22667261