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| AMP: The early Universe | ||||
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The Universe evolved from a fully-ionized plasma to an almost neutral
state in which molecules could form and the first stars were created. We
are engaged in studies of the atomic and molecular processes that took place
and were crucial to the formation of structure. (A.Dalgarno, Molecular
Processesin the Early Universe, J. Phys. Conf. Series 4, 10, 2005;
The Growth of
Molecular Complexity in the Universe, Faraday Discuss. 133, 9, 2006).
Project Links
People
A. Dalgarno and collaborators |
Brightness distribution of the charge-exchange X-ray emission induced by
the solar wind,
interacting with the interstellar neutral gas. | ||
