MASS GALAXIES
The search for active black holes in nearby low mass galaxies using optical and mid IR data
... dwarf galaxies and confirm the AGN nature of the ...star-forming galaxies, then this could further explain the bluer colours observed in these objects compared to the optically selected ...
21
Effects of AGN feedback on ΛCDM galaxies
... of galaxies by using a combination of a cosmological N-body simulation of the concordance Lambda cold dark matter (CDM) paradigm and a semi-analytic model of galaxy ...BH mass and mass, velocity ...
16
Stellar mass function of cluster galaxies at z ~ 1 5: evidence for reduced quenching efficiency at high redshift
... quenched galaxies compared to the field, even slightly before this epoch ...on galaxies from protoclusters to ma- ture clusters, we need to study large and, to the extent possi- ble, homogeneously-observed ...
13
The ACS Virgo Cluster Survey XV The Formation Efficiencies of Globular Clusters in Early Type Galaxies: The Effects of Mass and Environment
... Another plausible explanation is that the environment plays an important role in quenching the later, lower level star formation that builds up the field. Ram pressure stripping of gas will be more efficient in ...
28
Abundance ratios of red giants in low mass ultra faint dwarf spheroidal galaxies
... many galaxies of the Local Group using 10-m class telescopes and medium-resolution spectroscopy at the level of R ' 8000 and ...these galaxies as entities, but we can also check for the universality of the ...
13
Mass and star formation rate evolution of infrared selected galaxies in the COSMOS field = Evolución de la masa y de la tasa de formación estelar de galaxias seleccionadas en el infrarrojo en el campo COSMOS
... massive galaxies have older stellar populations and formed their stars earlier and more rapidly than low mass ...spiral galaxies of intermediate mass into blue quiescent and successively into ...
191
A NuSTAR survey of nearby ultraluminous infrared galaxies
... intrinsic 2 – 10 keV luminosity, developed from samples of Seyfert galaxies, may not be appropriate for ULIRGs. We thank Lee Armus who provided useful comments in the early planning phase of the NuSTAR ULIRG ...
16
Metodología para implementación de mass customization
... de Mass Customization para esta empresa se propone desarrollar un configurador de producto a través del cual el agente de ventas o el cliente (si se desea eliminar al intermediario) introducen sus requerimientos y ...
82
MASS SCHEDULE / HORARIO DE MISAS
... A causa de la fideli- dad del pueblo de Dios, y de la fide- lidad de Dios para ellos, todos los pueblos serán hijos de Dios y se regocijarán en el cumplimiento de la promesa de Dios a[r] ...
7
Distant galaxies analysis with deep neural networks
... • Design and training of 4 different neural networks • Prediction of Redshift, Stellarity, Stellar Mass and Spectral Type of galaxies • Data from Alhambra Survey • Comparison of Predicte[r] ...
31
A geometrical model for the catalogs of galaxies
... Cosmological N -body: Through N -body ex- periments by Aarseth (1978) it is possible to simulate groups which are analogous to the groups among bright Zwicky-catalog galaxies, see Turner et al. (1979) or ...
20
Environmental Effects on the physical properties of galaxies: Clues to the formation of S0 galaxies
... nearby galaxies. To solve this problem, the isophotes of cD galaxies were modeled by ellipses and subtracted from the original frames by Brown ...cD galaxies, the adoption of the strategies discussed ...
229
ON THE CLUSTERING OF SUBMILLIMETER GALAXIES
... In terms of the results of previous studies of SMG clustering, direct comparisons are difficult to make because of the differing wavelengths and flux limits of each survey. Poorly quantified redshift distributions in all ...
9
Propuesta para una Antropología de los Mass Media
... los mass media es un campo dentro de la antropología que trata de la relación entre los medios masivos de comunicación y la ...los mass media dice que nosotros estamos interesados en cómo una manera de ser ...
11
A possible origin of the mass metallicity relation of galaxies
... dian mass–metallicity ...for galaxies with strongly fluctuating star formation ...steeper mass–metallicity relation would be achieved than the ones produced by either process ...dwarf ...
12
ON THE EQUILIBRIUM OF A DISTORTED HETEROGENEOUS ELLIPSOIDAL MASS. III: THE HETEROGENEOUS SPHEROIDAL MASS
... In the case of our heterogeneous mass, equa- tion (46) is not acceptable, especially at points where external potentials are needed (they must approach 0, as r → ∞ ). To obtain equilibrium figures for the ...
9
Newborn mass screening and selective screening using electrospray tandem mass spectrometry in Japan
... tandem mass spectrometry was applied to detect a series of inherited metabolic disorders during a newborn-screening pilot study and a selective screening in ...our mass screening of 102 200 newborns, five ...
10
A Chandra Perspective on Galaxy Wide X ray Binary Emission and its Correlation with Star Formation Rate and Stellar Mass: New Results from Luminous Infrared Galaxies
... nents that were undetected in the 2–8 keV band. For NGC 23, the nucleus was detected in the 2–8 keV band, but due to the increased background over the larger galaxy-wide area, the total galaxy emission was formally ...
13
Code for Interpreters Mass Court
... If the court agrees that the error could be prejudicial, then the court shall hear evidence as to what the correct interpretation should be from information submitted by both counsels,[r] ...
7
Ly alpha EMITTING GALAXIES AT z=2 1 IN ECDF S: BUILDING BLOCKS OF TYPICAL PRESENT DAY GALAXIES?
... conditional mass function to predict the expected bias evolution as a function of redshift (Figure ...the mass distribution of descendants for a family of dark matter halo masses at high ...conditional ...
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