Special Session 7 Young Stars, Brown Dwarfs, and Protoplanetary Disks
Abstract
In recent years our knowledge of star, brown dwarf and planet formation has progressed immensely due to new data in the IR domain (Spitzer telescope), new X-ray campaigns such as the Chandra Orion Ultradeep Project (COUP) and the X-ray Emission Survey of Taurus (XEST), with XMM-Newton, as well as adaptive optics results and synoptic studies of young stellar and substellar objects.
- Publication:
-
Highlights of Astronomy
- Pub Date:
- November 2010
- DOI:
- 10.1017/S1743921310011191
- Bibcode:
- 2010HiA....15..727G