Galactic Structure Model and Intracluster Contamination
Studies of the Structure and Evolution of the Intracluster Medium
... merger model where the trajecto ry lies approxim ately 65° out of the plane of th e sky, and a t this viewing angle it becomes even more challenging to make quantitative statem ents abo u t th e ICM properties ...
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Structure of brightest cluster galaxies and intracluster light
... This method is suitable when the dither pattern is larger than the target. Hence, suffi- cient sky coverage is available to model the average background pattern. In the first step an intermediate stack is created ...
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Galactic Structure and Holography
... Abstract Galactic structure, involving bulk motion of matter conserving mass and an- gular momentum, is analyzed in a holographic large scale structure ...
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Gravitational Description and Graphics of a Wormhole Structure—A Galactic Megamaximon
... In this paper, we describe this solution, show the procedure of a wormhole occurrence analytically and graphically, and apply this model to study the possi- How to cite this paper: Khlestkov, Yu.A., Lukashina, ...
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An investigation of galactic structure made from the study of the northern hemisphere early type stars at intermediate galactic latitudes
... light from the diaphragm . This splits the light into two beams, the ratio of the intensities of the two beams being dependent on the choice of beam splitter. Initially a 50-50 beam splitter was used, but this was ...
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Structure in the polarized Galactic synchrotron emission, in particular ``depolarization canals''
... from Eq. (3). Both predictions have arbitrary polarized intensi- ties. Therefore, the scaling of the models contains no physical information, and is adjusted to fit the data. The accuracy of the model predictions ...
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Interaction of Hydra A Jets with the Intracluster Medium
... radio structure of Hydra A, we aimed to constrain the jet precession period and the precession angle, and explain in detail the jets interaction with the cluster ...axisymmetric model to a three dimensional ...
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Planck intermediate results XLIV Structure of the Galactic magnetic field from dust polarization maps of the southern Galactic cap
... density structure and the e ff ective correlation length of the GMF contribute to the large dispersion of p observed in the ...high Galactic latitudes will be to fit the E and B power ...our model to ...
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Unveiling the Structure of Active Galactic Nuclei with Hard X ray Spectroscopy
... this model: 93 targets (82 %, excluding unobscured sources) reach p null > 5 % for the best-fit set of ...the model does not provide a good fit to the ...MYtorus model is a pile-up of best-fit ...
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The environmental dependence of the structure of galactic discs in STAGES S0 galaxies: implications for S0 formation
... Systematic errors in scalelength due to the error in the sky subtraction are also typically < 10 per cent. Contamination of the cluster sample by the field is < 25 per cent. We find no significant difference ...
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Model Number Structure
... The following are some examples of applications for which particular attention must be given. This is not intended to be an exhaustive list of all possible uses of the products, nor is it intended to imply that the uses ...
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Model Number Structure
... The following are some examples of applications for which particular attention must be given. This is not intended to be an exhaustive list of all possible uses of the products, nor is it intended to imply that the uses ...
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Time but no space : resolving the structure and dynamics of active galactic nuclei using time domain astronomy
... toy model in which asymmetric broad lines arise by a mis- aligned inner-and-outer accretion disc system that asymmetrically heats the ...disc structure with a tearing radius due to the different spins of ...
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Local galactic structure
... result of this investigation has been that the interstellar medium consists largely of expanding HI bubbles of a variety of dim e nsions. These bubbl es are though[r] ...
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A multiphase model of galactic collapse
... ra tio s a n d to o m an y black holes. An a lte rn a tiv e solution is th a t oxygen is p re fe re n tia lly rem oved from th e system by a galactic w ind. T h e th ic k disk provides a possible site of th e o u ...
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Structure and mass segregation in Galactic stellar clusters
... their structure and mass segregation levels with those derived from numerical ...the structure of the nascent clusters and can follow the evolution of the cluster properties during its build ...
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Characteristics of the structure in the Galactic polarized radio background at 350 MHz
... and structure functions of the Stokes parameters Q and U and polarized intensity P are derived from three sets of radio polarimetric ...and structure functions of rotation measure RM as ...over ...
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Pulsating variable stars as tracers of galactic structure and interaction mechanisms
... CMD, structure and distance to Leo IV Figure ...the Galactic GC M15 (from Durrell & Harris 1993; solid line) properly shifted in magnitude and color, and selected as stars most likely belonging to the ...
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Fast Galactic Structure Finding using Graphics Processing Units
... scale structure forma- tion and galaxy evolution. Structure finding, that is, the discovery of gravitationally-bound objects such as dark matter halos, is a crucial step in many such ...
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A high resolution picture of the intracluster gas
... Among the first Chandra cluster results was a discovery of “cold fronts” in merg- ing clusters A2142 and A3667 (Markevitch et al. Figure 2 shows ACIS images of A2142 and A3667 with promi[r] ...
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