The BIMA millimeter wave array has provided maps of the young star forming region around SVS13 on angular scales from 0.2" to 100". Disks and envelopes around the two principal objects in the region are resolved, allowing simple models of both to be constructed. Differences in the emission spectra between each disk and its envelope suggest early grain growth in the disks.
Friday, 27 April 2001
11:00am
Array Operations Center Auditorium
Local Host: Rick Perley