ALMA detection of a tentative nearly edge-on rotating disk around the nearby AGB star R Doradus
Abstract
A spectral scan of the circumstellar environment of the asymptotic giant branch (AGB) star R Doradus was taken with ALMA in cycle 2 at frequencies between 335 and 362 GHz and with a spatial resolution of 150 milliarcseconds. Many molecular lines show a spatial offset between the blue and red shifted emission in the innermost regions of the wind. The position-velocity diagrams of this feature, in combination with previous SPHERE data and theoretical work point towards the presence of a compact differentially rotating disk, orientated nearly edge-on. We model the 28SiO (v = 1, J = 8 → 7) emission with a disk model. We estimate the disk mass and angular momentum to be 3 × 10-6 M⊙ and 5 × 1040 m2 kg s-1. The latter presents an "angular momentum problem" that may be solved by assuming that the disk is the result of wind-companion interactions with a companion of at least 2.5 earth masses, located at 6 AU, the tentatively determined location of the disk's inner rim. An isolated clump of emission is detected to the south-east with a velocity that is high compared to the previously determined terminal velocity of the wind. Its position and mean velocity suggest that it may be associated with a companion planet, located at the disk's inner rim.
- Publication:
-
Astronomy and Astrophysics
- Pub Date:
- June 2018
- DOI:
- 10.1051/0004-6361/201732246
- arXiv:
- arXiv:1803.06207
- Bibcode:
- 2018A&A...614A.113H
- Keywords:
-
- radiative transfer;
- stars: AGB and post-AGB;
- circumstellar matter;
- submillimeter: stars;
- Astrophysics - Solar and Stellar Astrophysics
- E-Print:
- 11 pages, 7 Figures