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Infrared-luminous galaxies

An obvious way of testing such ideas is to see how the number and properties of infrared-luminous galaxies vary with redshift as we probe back into time. R infrared activity is in fact triggered by galaxy-galaxy interactions. [Pg.273]

Radiation in the far IR from either cool dust associated with cirrus or warm dust associated with active star formation in luminous and ultra-luminous infrared galaxies. [Pg.396]

The strongly evolving population of Luminous Infrared Galaxies suggesting that they are progenitors of massive spheroidals (Blain et al. 1999 Elbaz et al. 1999). [Pg.239]

Fig. 7.15 Color composite image of ultra-luminous infrared galaxy IRAS... Fig. 7.15 Color composite image of ultra-luminous infrared galaxy IRAS...
See other pages where Infrared-luminous galaxies is mentioned: [Pg.273]    [Pg.561]    [Pg.273]    [Pg.561]    [Pg.139]    [Pg.274]    [Pg.523]    [Pg.87]    [Pg.370]    [Pg.377]    [Pg.379]    [Pg.13]    [Pg.204]    [Pg.47]    [Pg.146]    [Pg.148]    [Pg.160]    [Pg.117]    [Pg.139]    [Pg.140]   
See also in sourсe #XX -- [ Pg.269 ]



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Galaxie

Infrared galaxies

Luminous

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