VI/147          Galaxies Chemical and photometric evolution models (Molla, 2014)

Chemical and photometric evolution models for disk, irregular, and low mass galaxies. Molla M. <Advances in Astronomy, vol. 2014, id.162949 (2014)> =2014AdAst2014E..13M 2014AdAst2014E..13M =2015yCat.6147....0M 2015yCat.6147....0M
ADC_Keywords: Models, evolutionary ; Galaxies, photometry ; Abundances Keywords: galaxies: evolution - galaxies: spiral - galaxies: low mass - galaxies: abundances - galaxies: photometry - galaxies: evolution Abstract: We summarize the updated set of multiphase chemical evolution models performed with 44 theoretical radial mass initial distributions and 10 possible values of efficiencies to form molecular clouds and stars. We present the results about the infall rate histories, the formation of the disk, and the evolution of the radial distributions of diffuse and molecular gas surface density, stellar profile, star formation rate surface density, and elemental abundances of C, N, O, and Fe, finding that the radial gradients for these elements begin steeper and flatten with increasing time or decreasing redshift, although the outer disks always show a certain flattening for all times. With the resulting star formation and enrichment histories, we calculate the spectral energy distributions (SEDs) for each radial region by using the ones for single stellar populations resulting from the evolutive synthesis model POPSTAR. With these SEDs we may compute finally the broad band magnitudes and colors radial distributions in the Johnson and in the SLOAN/SDSS systems which are the main result of this work. We present the evolution of these brightness and color profiles with the redshift. Description: These tables give the theoretical chemical and photometric evolution of galaxies from the cited paper. Basically give tables 2, 3 and 4 for the 440 models from Molla & Diaz (2005, Cat. J/MNRAS/358/521) and Molla (2014AdAst2014E..13M 2014AdAst2014E..13M). These models correspond to 44 different galaxy dynamical mass defined by a number between 1 and 44 (see Table 1 from Molla & Diaz (2005, J/MNRAS/358/521) where properties for each of these theoretical galaxy mass distributions are given). For each one 10 different values of efficiences to form molecular clouds and stars are used (see Table 2 from Molla & Diaz 2005, Cat. J/MNRAS/358/521). Tables 2 and 3 refer to the chemical evolution results, while table 4 give the photometric evolution. All tables give the evolution of the different radial regions of theoretical galaxies, this way it is necessary to integrate these results to obtain the evolution of a galaxy as a whole. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file list.dat 46 440 List of available files table2/* . 440 *Evolution of different phases of mass in each radial region of a galaxy starting in t=0 for a total of 1297 time steps table2bis/* . 440 *Evolution of different phases of mass in each radial region of a galaxy. Continuation table3/* . 440 *Evolution of Abundances y mass for 14 elements for each radial region of a galaxy starting in t=0 for a total of 1297 time steps table3bis/* . 440 *Evolution of Abundances y mass for 14 elements for each radial region of a galaxy. Continuation table4/* . 440 *Evolution of absolute magnitudes for 12 bands in the Johnson system and 5 in the SLOAN/SDSS system starting in t=0.010 (one time step less than the other tables) -------------------------------------------------------------------------------- Note on table*: files named table*/table*xxyy.dat, xx means the type of efficiency, between 01 and 10 and yy means the number of the total mass distribution, between 01 and 44. -------------------------------------------------------------------------------- See also: J/MNRAS/358/521 : Galaxies grid of chemical evolution models (Molla+, 2005) Byte-by-byte Description of file: list.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 2 I02 --- nt [01/10] Type of efficiency 4- 5 I02 --- dis [01/44] Number of the total mass distribution 7- 12 A6 --- T2 Link to the table in subdirectory table2 for evolution of different phases of mass 14- 22 A9 --- T2bis Link to the table in subdirectory table2bis for evolution of different phases of mass 24- 29 A6 --- T3 Link to the table in subdirectory table3 for Evolution of Abundances y mass for 14 elements 31- 39 A9 --- T3bis Link to the table in subdirectory table3bis for Evolution of Abundances y mass for 14 elements 41- 46 A6 --- T4 Lint to the table in subdirectory table4 for evolution of absolute magnitudes for 12 bands in the Johnson system and 5 in the SLOAN/SDSS system -------------------------------------------------------------------------------- Byte-by-byte Description of file (# headlines): table2/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 11 E10.5 Gyr t Time 13- 17 F5.3 --- z redshift computed from MacDonald (2006, Foundations of Physics Letters, vol. 19, 631) with a delay t0=0.6Gyr to start to form galaxies 19- 20 I2 kpc r Galactocentric Radius of each radial region 23- 32 E10.5 Msun/yr SFRh SFR in the halo radial region multiplied by 10 35- 44 E10.5 Msun/yr SFRd SFR in the disk radial region multiplied by 10 47- 56 E10.5 10+9Msun Mh Mass in the halo radial region 59- 68 E10.5 10+9Msun Md Mass in the disk radial region -------------------------------------------------------------------------------- Byte-by-byte Description of file (#): table2bis/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 11 E10.5 10+9Msun gh Mass in the diffuse gas phase in the halo region 14- 23 E10.5 10+9Msun s1h Mass in the low mass and intermediate stellar mass phase in the halo region 26- 35 E10.5 10+9Msun s2h Mass in the massive stellar mass phase in the halo region 38- 47 E10.5 10+9Msun remh Mass in the remnant phase in the halo region 50- 59 E10.5 10+9Msun g Mass in the diffuse gas phase in the disk region 62- 71 E10.5 10+9Msun c Mass in the molecular gas phase in the disk region 74- 83 E10.5 10+9Msun s1 Mass in the low mass stellar phase in the disk region 86- 95 E10.5 10+9Msun s2 Mass in the massive stellar phase in the disk region 98-107 E10.5 10+9Msun rem Mass in the remnant phase in the disk region -------------------------------------------------------------------------------- Byte-by-byte Description of file (#): table3/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 11 E10.5 Gyr t Time 13- 17 F5.3 --- z Redshift 19- 20 I2 kpc r Galactocentric radius 23- 32 E10.5 --- H Abundance of H in each radial region of the disk as mass proportion 35- 44 E10.5 --- D Abundance of D in each radial region of the disk as mass proportion 47- 56 E10.5 --- 3He Abundance of He3 in each radial region of the disk as mass proportion 59- 68 E10.5 --- 4He Abundance of He4 in each radial region of the disk as mass proportion -------------------------------------------------------------------------------- Byte-by-byte Description of file (# headlines): table3bis/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 2- 11 E10.5 --- C12 Abundance of C12 in each radial region of the disk as mass proportion 13- 23 E11.5 --- C13 Abundance of C13 in each radial region of the disk as mass proportion 26- 35 E10.5 --- N Abundance of N in each radial region of the disk as mass proportion 38- 47 E10.5 --- O Abundance of O in each radial region of the disk as mass proportion 50- 59 E10.5 --- Ne Abundance of Ne in each radial region of the disk as mass proportion 62- 71 E10.5 --- Mg Abundance of Mg in each radial region of the disk as mass proportion 74- 83 E10.5 --- Si Abundance of Si in each radial region of the disk as mass proportion 86- 95 E10.5 --- S Abundance of S in each radial region of the disk as mass proportion 98-107 E10.5 --- Ca Abundance of Ca in each radial region of the disk as mass proportion 110-119 E10.5 --- Fe Abundance of Fe in each radial region of the disk as mass proportion -------------------------------------------------------------------------------- Byte-by-byte Description of file (#): table4/* -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 4 I2 --- Nt Number defining the efficiencies set to form molecular clouds and stars 9- 10 I2 --- Ndis Number defining the total radial mass distribution 13- 16 I4 --- Ngen Number of the evolutionary step or generation of star formation 20- 25 F6.3 Gyr Time Evolutionary Time 30- 34 F5.3 --- z Redshift 38- 41 F4.1 kpc r Galactocentric Radius in kpc 44- 50 E7.2 pc+2 A1 Surface of the ring at the galactocentric radius 53- 59 E7.2 pc+2 A2 Surface of the disk at the same galactocentric radius 63- 71 E9.4 mag UV1MAG Absolute magnitude of the Ultraviolet filter f130m of HST 73- 81 E9.4 mag UV2MAG Absolute magnitude of the Ultraviolet filter f210m of HST 83- 91 E9.4 mag UMAG Absolute magnitude of the U Johnson filter 93-101 E9.4 mag B1MAG Absolute magnitude of the B Johnson filter for U-B 103-111 E9.4 mag B2MAG Absolute magnitude of the B Johnson filter for B-V 113-121 E9.4 mag VMAG Absolute magnitude of the V Johnson filter 123-131 E9.4 mag RMAG Absolute magnitude of the R Johnson filter 133-141 E9.4 mag IMAG Absolute magnitude of the I Johnson filter 143-151 E9.4 mag JMAG Absolute magnitude of the J Johnson filter 153-161 E9.4 mag HMAG Absolute magnitude of the H Johnson filter 163-171 E9.4 mag KMAG Absolute magnitude of the K Johnson filter 173-181 E9.4 mag LMAG Absolute magnitude of the L Johnson filter 183-191 E9.4 mag uMAG Absolute magnitude of the u SOAN/SDSS filter 193-201 E9.4 mag gMAG Absolute magnitude of the g SOAN/SDSS filter 203-211 E9.4 mag rMAG Absolute magnitude of the r SOAN/SDSS filter 213-221 E9.4 mag iMAG Absolute magnitude of the i SOAN/SDSS filter 223-231 E9.4 mag zMAG Absolute magnitude of the z SOAN/SDSS filter -------------------------------------------------------------------------------- Acknowledgements: Mercedes Molla, mercedes.molla(at)ciemat.es
(End) Patricia Vannier [CDS] 01-Dec-2015
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