High Angular Resolution Studies of Disks-the Millimetre

Details High Angular Resolution Studies of Disks-the Millimetre High Angular Resolution Studies of Disks-the Millimetre

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004iaus..221..381w&link_type=abstract

Star Formation at High Angular Resolution, International Astronomical Union Symposium 221, held during the XXV General Assembly

Astronomy and Astrophysics

Astronomy

Scientific paper

I briefly review progress in high angular resolution observations of disks at millimetre wavelengths, with a focus on dust continuum observations of the disks surrounding low mass pre-main-sequence stars. I summarize the utility of observations at millimetre wavelengths, where dust emission is largely optically thin, and I touch on several recent directions, including imaging surveys using interferometers, testing physical models of disks with resolved observations, and the complexities introduced by stellar multiplicity.

Affiliated with

Also associated with

No associations

Rating

High Angular Resolution Studies of Disks-the Millimetre 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 High Angular Resolution Studies of Disks-the Millimetre, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High Angular Resolution Studies of Disks-the Millimetre will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-796751