[PDF] Top 20 Evolution of star-forming dwarf galaxies: characterizing the star formation scenarios

... number of models have computed purely chemical evolution mod- els for BCDs or dIrr galaxies (Chiosi & Matteucci 1982; Marconi, Matteucci & Tosi 1994; Recchi et ...Most of them assume ... See full document

... number of models have computed purely chemical evolution mod- els for BCDs or dIrr galaxies (Chiosi & Matteucci 1982; Marconi, Matteucci & Tosi 1994; Recchi et ...Most of them assume ... See full document

... majority of our individual spectra, which were reduced to zero redshift, have S/N ratios per ...to the detec- ˚ tion of small equivalent width [OII] emission, which is expected to be found in bulge ... See full document

... paths of AGN growth. On one path, AGN growth and host star formation are tightly coupled by an evolutionary mechanism, likely ...in the diagonal correlation line in Fig. 6. The other ... See full document

... consider the possible role of AGN feedback in the evolution of late-type ...galaxies. The majority of black holes grow- ing locally and at high redshift are hosted ... See full document

... MS galaxies and X-ray AGN hosts suggest that the radio-excess characteristic of our sources is not only due to a stronger radio core emission from the AGN than in “radio-normal” sources, but ... See full document

... mimic the star formation histories we insert the star clusters at different times into the ...different star formation histories. Figure 3.1 shows the SFHs ... See full document

... possible scenarios. ( 1 ) One star in the binary has a  mass  ..., the other star is more massive and evolves into a white dwarf fi rst, and then the white dwarf ... See full document

... that the merging of comparable mass systems is what produces the large luminosities found in the SMG population ...One of the reasons is the irregular complex morphologies ... See full document

... relation of SFR surface density ...within galaxies. The plot is adopted from Figure 1 of Elmegreen ( 2015 ) , with the SFRs for the LSF and HSF regions of NGC 3738 and DDO ... See full document

... One of the most important goals of modern astrophysics is to understand the forma- tion and evolution of the universe and the structures it ...1996 the ... See full document

... understand the cosmic history of star formation and black hole growth, we must understand infrared (IR) emission; the more in- tense the star formation, the ... See full document

... function of gross galaxy prop- erties (Saintonge et ...level of disturbance and offset from the so-called Galaxy Main Sequence of star formation ...host galaxies have ... See full document

... reveals the knee for both populations. This fact allows us to compare the level of [ X / Fe ] in stars from each population formed before and after the main contribution of SN Ia to ... See full document

... measurements of the space density as a function of luminosity (triangles) together with the expectations from three different z = 0 CT AGN luminosity functions: Della Ceca et ...For the ... See full document

... NSC formation: (1) globu- lar clusters which collect at the center due to dynamical friction ( Tremaine et ...cretion of gas onto the center followed by in situ star formation ( ... See full document

... With the new identifica- tions, the total number of X-shaped radio galaxies spectroscop- ically identified is increased to ...60. The last object of our sam- ple, J1258 + 3227, ... See full document

... that the distribution of points is not symmetrical about the one-to-one line as would be expected if both primary and secondary responded equally to the tidal ...overpopulation of ... See full document

... extinction. The systematic uncertainties which arise from the choice of stellar evolution model, IMF, and extinction law can be large and often exceed the statistical uncertainties from ... See full document

... sources) of the VLA and GMRT ...reduce the influence of radio-loud AGNs. We adopt the weighted average method to be consistent with the analysis in other wavebands, and we adopt ... See full document