Galaxy: Structure
Dynamical structure of the molecular interstellar medium in an extremely bright, multiply lensed z 3 submillimeter galaxy discovered with Herschel
... velocity structure of the gas reservoir suggests that the brightest two lensed images are dynamically resolved projections of the same dust-obscured region in the galaxy that are kinematically offset from ...
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Alignments of galaxy group shapes with large scale structure
... between galaxy group shapes and the surrounding galaxy distribution in both, real galaxy groups obtained from the Sloan Digital Sky Survey Data Release 7 (SDSS-DR7, Abazajian et ...between ...
11
The age structure of globular cluster systems in early type galaxies and its dependence on host galaxy properties
... age structure, as represented by the Methuselah parameter, and var- ious host galaxy parameters, our current galaxy sample is a first step towards probing the range of host galaxy parameters ...
10
The representative XMM Newton cluster structure survey (REXCESS) of an X ray luminosity selected galaxy cluster sample
... 63 galaxy clusters in the sky away from galactic plane, the HIFLUGCS sample (Reiprich & Böhringer 2002), providing an account at even lower redshifts (although with a somewhat less ideal field-of-view ...
15
Galaxy interactions II High density environments
... of galaxy-galaxy interactions and the role played by the global environment of the group on the properties of its number ...study galaxy interactions within groups and clusters with the aim of ...
9
Effects of superstructure environment on galaxy groups
... the galaxy properties, such as the star formation rate (SFR) or galaxy colours, also depend on large-scale structure (Binggeli 1982; Donoso, O’Mill & Lambas 2006; Crain et ...2dF Galaxy ...
8
OPPL-Galaxy, a Galaxy tool for enhancing ontology exploitation as part of bioinformatics workflows
... Ontology debugging (the process of fixing defects in an ontology) can be a daunting activity, especially when the ontology the scientist is working with has not been developed in-house and/or if it presents a complex ...
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Effects of superstructure environment on galaxy groups
... One of the largest and most ambitious surveys carried out so far is the Sloan Digital Sky Survey (York et al. 2000). It has deep multi- color images covering more than one quarter of the sky and cre- ates ...
8
The metallicity and dust content of a redshift 5 gamma ray burst host galaxy
... The low- and high-ionization lines show multiple compo- nents. Due to their saturation, we do not include the Si iv and C iv lines in our analysis. The absorption lines from singly ion- ized species are fitted with Voigt ...
12
THE ADVANCED CAMERA FOR SURVEYS FORNAX CLUSTER SURVEY VII HALF LIGHT RADII OF GLOBULAR CLUSTERS IN EARLY TYPE GALAXIES
... Sombrero galaxy (Spitler et ...host galaxy luminosity are encompassed by the work on dwarf galaxies by Georgiev et ...SB0 galaxy NGC 1533 in the Dorado ...host galaxy morphologies and ...
19
Galaxy star formation in different environments
... red galaxy fractions using samples of galaxies located at different halo/void centric distances at fixed local densities (the different samples are defined in the previous subsection, ...red galaxy fraction ...
12
ALMA Observations of Gas rich Galaxies in z ~ 1 6 Galaxy Clusters: Evidence for Higher Gas Fractions in High density Environments
... Galaxy cluster evolution is intertwined with that of its constituent galaxies. Therefore, in order to understand the former, we must explore the baryonic processes that shape the latter. In particular, this ...
6
Ages and Heavy Element Abundances from Very Metal poor Stars in the Sagittarius Dwarf Galaxy
... Sagittarius ( Sgr ) is a massive disrupted dwarf spheroidal galaxy in the Milky Way halo that has undergone several stripping events. Previous chemical studies were restricted mainly to a few, metal-rich ([ Fe / H ...
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SDSS IV MaNGA: Dependence of Global and Spatially Resolved SFR M ∗ Relations on Galaxy Properties
... Σ Hα ( H II )–Σ * ( H II ) relation driven by star formation alone. The result is presented in Figure 2 ( b ) . For the star-forming regions, Σ Hα ( H II ) and Σ * ( H II ) are much more tightly correlated than that ...
8
How robust are predictions of galaxy clustering?
... the galaxy sample as a func- tion of halo mass, which takes into account the halo mass function and the halo ...central galaxy peak is much less distinct and satellite galaxies dominate the effective ...
14
Range structure analysis: Unveiling the internal structure of species' ranges
... RSA allows to identify specific locations, within the geo- graphic range of a species, where a given parameter is most important in driving spatial variation in occupancy dynamics (Fig. 2). In this particular example, ...
8
Cuentas anuales 2014 de la Red de Ciudades por la Bicicleta
... El activo no corriente esta formado por el Inmovilizado Material, que está compuesto por un ordenador y una impresora por importe de 773,85 euros. Este año se ha amortizado (dado a pérdidas) un teléfono Galaxy del ...
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Uncloaking globular clusters in the inner galaxy
... and ground data, whenever space-based observations deeper than ground-based observations exist, or the ground photometry in the rest of the cases. To quantify improvements in the photometry, we have measured the ...
45
Democracy in the age of media galaxy
... ABSTRACT – Representative democratic systems seem to be following divergent trends in recent times. On the one hand, there are certain signs of decline such as the fall in voter turnout or the increased distance between ...
16
Global environmental effects versus galaxy interactions
... of galaxy cluster where systems interact at low velocities, resembling galaxy interactions occur- ring within groups, falling along cluster ...where galaxy interactions are more frequent, low ram ...
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