[PDF] Top 20 Galaxy and Mass Assembly (GAMA): the star formation rate dependence of the stellar initial mass function
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Galaxy and Mass Assembly (GAMA): the star formation rate dependence of the stellar initial mass function
... of star formation. This initial stellar mass distribu- tion has often been assumed to be ...all galaxy formation and evolution ...low mass stars, which form the ... See full document
16
Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
... Large galaxy surveys have also been a driving force in the field of galaxy evolution, although for a different ...structure formation appears well understood, our theoretical understanding of the ... See full document
40
Galaxy and Mass Assembly (GAMA): the red fraction and radial distribution of satellite galaxies
... the Galaxy And Mass Assembly ...account stellar mass estimates, we find 3514 isolated galaxies of which 1426 host a total of 2998 ...a function of satellite mass, host ... See full document
13
GAMA/H ATLAS: common star formation rate indicators and their dependence on galaxy physical parameters
... indicators. GAMA provides a large sample of galaxies in the local Universe where photometric information in the UV and IR as well as measurements of key spec- tral lines such as H α and H β are ...our ... See full document
19
Galaxy And Mass Assembly (GAMA): end of survey report and data release 2
... Large galaxy surveys have also been a driving force in the field of galaxy evolution, although for a different ...structure formation appears well understood, our theoretical understanding of the ... See full document
40
The dependence of galaxy clustering on stellar mass, star formation rate and redshift at z = 0 8 − 2 2, with HiZELS
... the galaxy stellar mass function, and the galaxy-black hole mass ...(e.g. galaxy specific star- formation rate distributions, passive fractions and ... See full document
17
Galaxy and Mass Assembly (GAMA): morphological transformation of galaxies across the green valley
... the stellar population, ...the stellar population (Taylor et ...intrinsic stellar SED carried out in the optical for the GAMA sources (Taylor et ...in star formation rate, ... See full document
15
The origin of scatter in the star formation rate-stellar mass relation
... SFR, mass, dust attenuation and stellar ...fixed stellar mass (increasing the observed ...the galaxy lumi- nosity function, the redshift-comoving volume relation and the redshift ... See full document
18
Cosmic CARNage II: the evolution of the galaxy stellar mass function in observations and galaxy formation models
... the mass assembly of high-mass galaxies ...the galaxy stellar mass function over a range of ...Halo mass growth is the main driver of gas accretion rate in ... See full document
15
Guo, Qi (2009): Galaxy Formation and Evolution in a LCDM Universe. Dissertation, LMU München: Fakultät für Physik
... the initial stellar mass, are returned to the ...between star formation and SN explosions (both type I and type II), as well as the different heavy element yields associated with these ... See full document
141
Recycled stellar ejecta as fuel for star formation and implications for the origin of the galaxy mass-metallicity relation
... and Assembly of GaLaxies and their Environments and OverWhelmingly Large Simulations projects to assess the significance of recycled stellar ejecta as fuel for star ...of stellar ... See full document
24
Machine-learning-based photometric redshifts for galaxies of the ESO Kilo-Degree Survey data release 2
... r-band images. While magnitudes are measured in all filters, the star–galaxy separation, as well as the source positional and shape parameters, are based on the r-band data only. The choice of the r band as ... See full document
6
Slingshot prominence evolution for a solar like star
... solar-like star, we can calculate how the co-rotation and Alfv´en radii change with ...the star, but determining the Alfv´en radius is not an easy ...several stellar parameters currently not well ... See full document
6
Quenching or Bursting:the Role of Stellar Mass, Environment, and Specific Star Formation Rate to z ~ 1
... “stellar mass” of galax- ies and they often work together in the quench- ing mechanism (Peng et ...whereas mass quenching is mainly linked to centrals (Peng et ...of mass quenching and ... See full document
22
The triggering probability of radio-loud AGN: A comparison of high and low excitation radio galaxies in hosts of different colors
... a function of host galaxy stellar mass and radio luminosity ...law dependence typical for ...green galaxy population drops strongly, while in the blue pop- ulation it is ... See full document
7
Mapping the core mass function on to the stellar initial mass function: multiplicity matters
... It also suggests that most stars, including singles, are born in small groups of approximately four. This contrasts with the conclusion of Lada (2006) that most stars, being single, are born in isolation. In- ... See full document
10
Dynamical Masses of Young Star Clusters: Constraints on the Stellar IMF and Star-Formation Efficiency
... Fig. 1. Taken from [2]: Surface brightness profiles for three young clusters (left - M82-F, NGC 1569-A, and NGC 1705-1) and two N-body simulations which include the rapid removal of gas which was left over from a ... See full document
5
The energetics of starburst driven outflows at z ∼ 1 from KMOS
... energy rate is in agreement with the range of values using the first ...these mass outflow rates and kinetic energy estimates are similar to those derived for local starbursts using absorption line stud- ... See full document
15
Implications of a variable IMF for the interpretation of observations of galaxy populations
... simple stellar population depends on metallic- ...metallicity dependence of the metals released by individual stars, but the more significant contribution comes from the metallicity dependence of the ... See full document
15
Simulating the Milky Way is hard
... a mass of 10 5 M in the case of an L ∗ galaxy such as the Milky ...this mass, so each star particle represents more than 10 4 M ...a mass of stars would be comprised of multiple energy ... See full document
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