Searching for proto-brown dwarfs: Extending near IR spectroscopy of protostars below the hydrogen burning limitThe data presented herein were obtained at the W. M. Keck Observatory, which is operated as a scientific partnership among the California Institute of Technology, the University of California and the National Aeronautics and Space Administration. The Observatory was made possible by the generous financial support of the W. M. Keck Foundation.

Autor: T. P. Greene, G. W. Doppmann, C. J. Lada, B. A. Wilking
Zdroj: Astronomische Nachrichten; Dec2005, Vol. 326 Issue 10, p886-890, 0p
Databáze: Complementary Index
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