CO emission from high redshift

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dc.creatorGnedin, Nickolay Y.
dc.creatorSilk, Joseph
dc.creatorSpaans, Marco
dc.date2001-06-06
dc.date.accessioned2026-07-07T01:58:49Z
dc.date.available2026-07-07T01:58:49Z
dc.descriptionFuture 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.
dc.descriptionSubmitted to MNRAS
dc.identifierhttps://arxiv.org/abs/astro-ph/0106110
dc.identifierhttp://arxiv.org/abs/astro-ph/0106110
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/2869
dc.subjectAstrophysics
dc.titleCO emission from high redshift
dc.typetext

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