arXiv · astro-ph/9904173
CCS Imaging of the Starless Core L1544: An Envelope with Infall and Rotation
Abstract
We have carried out observations of the starless core L1544 in the CCS (J_N=3_2-2_1) line at 9 millimeters wavelength using the BIMA array. The maps show an elongated condensation, 0.15 x 0.045 pc in size, with stronger emission at the edges. The appearance is consistent with a flattened, ringlike structure viewed at high inclination to the line of sight. The CCS molecule is likely heavily depleted in the inner part of the core. The position velocity diagram along the major axis shows a remarkable pattern, a "tilted ellipse", that can be reproduced by a simple model ring with motions of both infall and rotation. The models suggest comparable velocities for infall and rotation, ~0.1 km/s, in the outermost envelope, at radius 15000 AU.
Explore related subjects
Keep this discovery
Explore connections, maps & timelines
Nagayoshi Ohashi, Siow Wang Lee, David J. Wilner, Masahiko Hayashi. 1999-04-13. CCS Imaging of the Starless Core L1544: An Envelope with Infall and Rotation. https://doi.org/10.1086/312067
Cite the original work for its findings. Save a collection to share your selection of sources.