CO emission from high redshift

Details CO emission from high redshift CO emission from high redshift

2001-06-06

arxiv.org/abs/astro-ph/0106110v1

Astronomy and Astrophysics

Astrophysics

Submitted to MNRAS

Scientific paper

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.

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