CO emission from high redshift
天体物理学
2007-05-23 v1
摘要
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.
引用
@article{arxiv.astro-ph/0106110,
title = {CO emission from high redshift},
author = {Nickolay Y. Gnedin and Joseph Silk and Marco Spaans},
journal= {arXiv preprint arXiv:astro-ph/0106110},
year = {2007}
}
备注
Submitted to MNRAS