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Special Session 7 Young Stars, Brown Dwarfs, and Protoplanetary Disks
Published online by Cambridge University Press: 21 October 2010
Extract
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.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 727 - 728
- Copyright
- Copyright © International Astronomical Union 2010