Observability of Early Evolutionary Phases of Galaxies at mm Wavelengths

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dc.creatorDe Zotti, G.
dc.creatorMazzei, P.
dc.creatorFranceschini, A.
dc.creatorDanese, L.
dc.date1996-02-29
dc.date.accessioned2026-07-07T02:20:57Z
dc.date.available2026-07-07T02:20:57Z
dc.descriptionSeveral lines of evidence and theoretical arguments suggest that a large fraction of starlight is absorbed by interstellar dust and re-radiated at far-IR wavelengths, particularly during early evolutionary phases of early type galaxies, which may even, under some circumstances, experience an optically thick phase. Therefore far-IR to mm observations are crucial to understand the galaxy evolution. The strong K-correction makes surveys at mm wavelengths ideally suited for studying high-$z$ galaxies. The broad redshift range covered by mm surveys at sub-mJy flux limits offers a good chance for gaining important information also on the geometry of the Universe.
dc.descriptionInvited review at the ESO IRAM NFRA Onsala Workshop "Science with Large Millimeter Arrays", Muenchen; tex file, 7 pages, 3 fig.s available on request
dc.identifierhttps://arxiv.org/abs/astro-ph/9602152
dc.identifierhttp://arxiv.org/abs/astro-ph/9602152
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/10384
dc.subjectAstrophysics
dc.titleObservability of Early Evolutionary Phases of Galaxies at mm Wavelengths
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