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- W3100412911 abstract "Aims. We study the analogy between local luminous and ultraluminous infrared galaxies (U/LIRGs) and high-z massive star forming galaxies (SFGs) by comparing their basic Hα structural characteristics, such as size and luminosity surface density, in an homoge- neous way (i.e. same tracer, size definition, and similar physical scales). Methods. We use integral field spectroscopy (IFS) based Hα emission maps for a representative sample of 54 local U/LIRGs (66 galax- ies) observed with INTEGRAL/WHT and VIMOS/VLT. From this initial sample, we select 26 objects with similar Hα luminosities (L(Hα)) to those of massive (i.e. M� ∼ 10 10 Mor larger) SFGs at z ∼ 2, and observed on similar physical scales. We then directly compare the sizes, and luminosity (and SFR) surface densities of these local and high-z samples. Results. The size of the Hα emitting region in the local U/LIRGs that we study has a wide range of values, with r1/2(Hα) from 0.2 kpc to 7 kpc. However, about two-thirds of local U/LIRGs with Lir > 10 11.4 Lhave compact Hα emission (i.e. r1/2 2 kpc). These are systems that show evidence of pre-coalescence merger activity and are indistinguishable from the massive high-z SFGs galaxies in terms of their Hα sizes, and luminosity and SFR surface densities." @default.
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- W3100412911 date "2012-05-01" @default.
- W3100412911 modified "2023-10-18" @default.
- W3100412911 title "Integral field spectroscopy based Hα sizes of local luminous and ultraluminous infrared galaxies. A direct comparison with high-z massive star-forming galaxies" @default.
- W3100412911 cites W1529348779 @default.
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- W3100412911 cites W1827714327 @default.
- W3100412911 cites W1914598719 @default.
- W3100412911 cites W1964925572 @default.
- W3100412911 cites W1973939397 @default.
- W3100412911 cites W1975777137 @default.
- W3100412911 cites W1977423663 @default.
- W3100412911 cites W1986761806 @default.
- W3100412911 cites W1988530166 @default.
- W3100412911 cites W1990491187 @default.
- W3100412911 cites W1994899031 @default.
- W3100412911 cites W1997032307 @default.
- W3100412911 cites W1997662069 @default.
- W3100412911 cites W1999299181 @default.
- W3100412911 cites W2000574072 @default.
- W3100412911 cites W2005531414 @default.
- W3100412911 cites W2011654732 @default.
- W3100412911 cites W2013575191 @default.
- W3100412911 cites W2016727820 @default.
- W3100412911 cites W2016829294 @default.
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