Galaxy Formation and Evolution: Low Surface Brightness Galaxies
Galaxy Formation and Evolution: Low Surface Brightness Galaxies
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DOI:
10.1046/j.1365-8711.1998.01731.x
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发表时间:
1998-04
影响因子:
4.8
通讯作者:
R. Jimenez;P. Padoan;F. Matteucci;A. Heavens
中科院分区:
文献类型:
--
作者:
R. Jimenez;P. Padoan;F. Matteucci;A. Heavens
ABSTRACT We investigatein detail the hypothesisthat low surfacebrightnessgalaxies(LSB) differfrom ordinary galaxies simply because they form in halos with large spin parameters.We compute star formation rates using the Schmidt law, assuming the same gas infalldependence on surface density as used in models of the Milky Way. We build stellarpopulation models, predicting colours, spectra, and chemical abundances. We compareour predictions with observed values of metallicity and colours for LSB galaxies andfind excellent agreement with all observables. In particular, integrated colours, colourgradients, surface brightness and metallicity match very well to the observed valuesof LSBs for models with ages larger than 7 Gyr and high values (λ > 0.05) for thespin parameter of the halos. We also compute the global star formation rate (SFR)in the Universe due to LSBs and show that it has a flatter evolution with redshiftthan the corresponding SFR for normal discs. We furthermore compare the evolutionin redshift of [Zn/H] for our models to those observed in Damped Lyman α systemsby Pettini et al. (1997) and show that Damped Lyman α systems abundances areconsistent with the predicted abundances at different radii for LSBs. Finally, we showhow the required late redshift of collapse of the halo may constrain the power spectrumof fluctuations.Key words: galaxies: formation – galaxies: evolution – galaxies: spiral – galaxies:stellar content.