Infrared galaxies in compact groups

Abstract IR properties of Compact Group (CG) galaxies are presented and compared with IR properties of isolated galaxies. Despite CGs displaying more E-S0s and optically bright galaxies, no differences are retrieved concerning FIR emission. The observed lack of strong FIR enhancement in the CG sampl...
Ausführliche Beschreibung

Gespeichert in:

Autor*in:	Kelm, B. [verfasserIn] Focardi, P. Zampieri, A.

Format:	Artikel
Sprache:	Englisch

Erschienen:	2003

Anmerkung:	© Kluwer Academic Publishers 2003

Übergeordnetes Werk:	Enthalten in: Astrophysics and space science - Kluwer Academic Publishers, 1968, 284(2003), 2 vom: Apr., Seite 471-474
Übergeordnetes Werk:	volume:284 ; year:2003 ; number:2 ; month:04 ; pages:471-474

Links:	Volltext

DOI / URN:	10.1023/A:1024043908361

Katalog-ID:	OLC2066236683

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abstract	Abstract IR properties of Compact Group (CG) galaxies are presented and compared with IR properties of isolated galaxies. Despite CGs displaying more E-S0s and optically bright galaxies, no differences are retrieved concerning FIR emission. The observed lack of strong FIR enhancement in the CG sample is not surprising when interpreting FIR sources in CGs as accordant redshift projections, rather than as mergers in progress. © Kluwer Academic Publishers 2003
abstractGer	Abstract IR properties of Compact Group (CG) galaxies are presented and compared with IR properties of isolated galaxies. Despite CGs displaying more E-S0s and optically bright galaxies, no differences are retrieved concerning FIR emission. The observed lack of strong FIR enhancement in the CG sample is not surprising when interpreting FIR sources in CGs as accordant redshift projections, rather than as mergers in progress. © Kluwer Academic Publishers 2003
abstract_unstemmed	Abstract IR properties of Compact Group (CG) galaxies are presented and compared with IR properties of isolated galaxies. Despite CGs displaying more E-S0s and optically bright galaxies, no differences are retrieved concerning FIR emission. The observed lack of strong FIR enhancement in the CG sample is not surprising when interpreting FIR sources in CGs as accordant redshift projections, rather than as mergers in progress. © Kluwer Academic Publishers 2003
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title_short	Infrared galaxies in compact groups
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