CO emission from high redshift

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Future observations with ALMA will be able to detect star-forming primordial gal axies, and perhaps even their dwarf spheroidal satellites, in CO emission lines at redshifts approaching 10. These observations will compliment other tools designed to study the dawn of galaxy formation, such as NGST and FIRST.
Submitted to MNRAS

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Astrophysics

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http://salesiana.dossiersoluciones.com/handle/123456789/2869

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/astro-ph/0106110
 http://arxiv.org/abs/astro-ph/0106110

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arXiv