Tidal stripping and disk kinematics in the RW Aurigae system

Details Tidal stripping and disk kinematics in the RW Aurigae system Tidal stripping and disk kinematics in the RW Aurigae system

Jun 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006a%26a...452..897c&link_type=abstract

Astronomy and Astrophysics, Volume 452, Issue 3, June IV 2006, pp.897-906

Astronomy and Astrophysics

Astrophysics

26

Stars: Individual: Rw Aur, Stars: Formation, Stars: Circumstellar Matter, Ism: Molecules, Radio Lines: Ism

Scientific paper

We present interferometric maps of the RW Aur system obtained with the IRAM Plateau de Bure Interferometer in CO(J=2-1), CO(J=1-0), and nearby continuum. The sub-arcsecond angular resolution (0.89''×0.58'') and high-sensitivity reached at 1.3 mm enable us to resolve three molecular structures: (1) an optically thick disk around RW Aur A in rotation about the optical jet axis, (2) a disturbed asymmetric peak around RW Aur B, (3) a 600 AU-long “arm” of material trailing from the RW Aur A disk. Comparison with Keplerian models indicates that the RW Aur A disk is the smallest detected so far around a T Tauri star (radius 40-57 AU) and that the CO emitting layer at the outer edge is warmer than the dust ({Tout}≃ 60-100 K) and relatively thick ({Nwarm}≃ 0.1-10×1022cm-2). The morphology and kinematics of the detected features strongly suggest that we are witnessing tidal stripping of the primary disk by the recent fly-by of RW Aur B. We speculate that tidal dissipation might explain the warmer gas temperatures in the RW Aur A disk compared with typical T Tauri stars, and perhaps play a role in its elevated accretion rate. We also find that the rotation sense of the RW Aur A disk is opposite to transverse velocity shifts in the optical jet reported by Woitas et al. (2005, A&A, 432, 149). We argue that these transverse shifts are likely to represent only upper limits to the true jet rotation speed. The limits remain consistent with current models of MHD launching from the disk.

Affiliated with

Also associated with

No associations

Rating

Tidal stripping and disk kinematics in the RW Aurigae system does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Tidal stripping and disk kinematics in the RW Aurigae system, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Tidal stripping and disk kinematics in the RW Aurigae system will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1854991