... Abstract: We present an extensive study of the radiative transfer in dusty galaxies based on Monte Carlo simulations. ... We have explored the dependence of A_l on a conspicuous set of quantities (Hubble type, inclination, dust optical thickness, dust distribution and extinction properties) for a large wavelength interval, ranging from 1250A to the K band, thus finally providing a comprehensive atlas of dust extinction in galaxies, which is electronically available. ... S04_MD20[ att , abs ] . ...

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• Clumpy dust disks
• The impact of Warm Dark Matter on the ages of galaxies
• Tracing Dust in Spiral Galaxies

Welcome to the Starburst and Galaxy Evolution website.

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• Our group
• Model Fitting
• Abstract

... Next: Cheating Poisson: A Up: Statistical Analysis Previous: Spatial Models and . ... The spatial distribution of stars in the Local Group dwarf irregular galaxy NGC 6822 has been studied, using recent positions and deep photometry for about 15,000 stars in the galaxy. Based on photometrical data, OB stars and red stars could be studied separately. Spatial statistical tools have been applied to the analysis of the spatial structure. ... Figure: Model selection by the aid of CAIC . ...

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• ADASS 2003 Conference Proceedings
• Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron
• Registering, PSF-Matching and Intensity-Matching Images in IRAF

... Science . ... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Properties of kinematically decoupled structures in Early-Type Galaxies . ... Science Users Information . ... ESO-MIDAS . ... ESO Science Newsletter . ... The project consists in measuring the stellar kinematics, stellar populations, dynamics, and morphological properties of the kinematically decoupled structures observed in the inner regions of Early-Type Galaxies. ... Return to list of thesis topics...

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• ESO - Thesis Topic: Dynamical models of multiple globular cluster populations
• ESO - Discs in Galaxies
• ESO - Thesis Topic: The interplay of massive stars, gas and dust in very nearby

... The sample of the Local Volume galaxies (distance smaller than 10 Mpc) gives a unique opportunity to study the properties of galaxies including the weakest objects: the absolute magnitude M B -10 and the virial mass M vir 10 9 M x263C;. ... Luminosity function of the Local Volume galaxies. ... The luminosity functions for galaxies are presented: red dashed line - from the 2dFGRS survey (Norberg et al. 2002); blue dash-dotted line - from the SDSS survey (Blanton et al. ...

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• New LBV Discovered in DDO 68 Galaxy
• Measurement of the dark halo shape in polar ring galaxies
• Galaxy sector, archive 2012

... Monday - November 21 (09:00h - 17:00h) . ... Welcome Tea Coffee . ... Session 1 (chair: Lister Staveley-Smith) . ... Morning Tea Coffee Session 2 (chair: Barbara Catinella) . ... Afternoon Tea Coffee Session 4 (chair: Guyla Jozsa) . ... Tuesday - November 22 (09:00h - 16:00h) Welcome Tea Coffee . ... Morning Tea Coffee Session 6 (chair: Ivy Wong) . ... Afternoon Tea Coffee . ... Wednesday - November 23 (09:00h - 16:00h) Welcome Tea Coffee . ... Morning Tea Coffee Session 9 (chair: Tom Jarrett) . ...

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• ATNF Daily Astronomy Picture
• WALLABY - the ASKAP HI All-Sky Survey
• Numerical Simulations of Galaxy Formation

... Astronomy for Kids . ... Astronomy 101 . ... Astronomy Day . ... Astronomy and astrophysics rely heavily on computer modeling, but being neither a physicist nor computer scientist, I cannot relate to the term "computer model." What is such a model, and how do scientists build one? ... Get instant access to subscriber content on Astronomy.com! ... If you are already registered on Astronomy.com, please log in below. ... Finescale Modeler | ... Model Railroader | Model Railroader Video Plus | ...

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• Besides computer simulations, what evidence do astronomers have to support the
• Understanding the Nice model | Astronomy.com
• Inside the cyclic model of the universe | Astronomy.com

. My astronomical research interests center on galaxy structure and evolution. Current topics include: . Polar-ring and interacting galaxies (see also new catalogue ) . Galaxy warps: statistics, properties and origin . Spiral galaxies at z~1: radial and vertical structure of stellar disks, statistics of interactions . Surface photometry and kinematics, dynamical modeling . Observational cosmology . Joomla Counter since Sep 1997

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• Database of Optical Properties
• Database of Optical Properties -- Level: subsubpage
• Database of Optical Properties -- Level: subpage

. Documents latest versions (PS and Latex)

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• Jonathan's ASC/SDS documents
• The AstroStat Slog model based
• The AstroStat Slog Blog Archive [MADS] multiscale modeling

... AstroGrid Registry . AstroGrid . 1.Home . 2.Admin Home . ... 1.Submit new resource . 2.Low Level(XML) Submit Resource . 3.Low Level(XML) Back Door Submit . ... 3.Get/Find New Registries . 4.Manage New Authority . 5.Remove Resource . ... 7.Resource(s) Status Change . ... 9.Admin Home (Other Tasks) . ... 8.Resource Help . ...

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• A 20 cm VLA survey of Abell clusters of galaxies
• The ROSAT AGN
• The very metal-poor local dwarf galaxies

... In this talk, I will discuss a study of the effect of ionization on the low end of HI mass function. The existence of a large population of low mass galaxies follows from CDM theory. ... HIDEEP found no low HI column density galaxies. One possible explanation is that the disks are "frozen". ... We assume that galaxies are exposed to an ionizing background radiation, from a uniform quasar distribution. ... We find a gap in the average column densities around N H which drops to 10 17 cm -2 . ...

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• Heiles Symposium Presentations
• Figures for Scattering Paper
• REU Science Area

... 2.3 Establishing the Extragalactic Distance Scale . ... 2.3.2 The Second Rung: Distances to stellar clusters . ... 2.3.4 Distances to Local Group Galaxies . ... The Luminosity Function of Planetary Nebulae . ... 3.2.2 Clusters of Galaxies . ... 4.2 Evidence for Dark Matter as a Function of Scale Size . ... 4.3 Other Dark Matter Indicators for Galaxies . ... What is the nature of the large-scale distribution of matter in the universe as traced by the three-dimensional galaxy distribution? ...

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• Physics 410/510 Observational Cosmology
• The Galaxy Gallery: Messier Objects
• Fabry-Perot Images of Interacting Galaxies

Galaxies follow tight scaling relations linking their dynamical properties to their baryonic content. The study of these dynamical laws strongly constrains cosmological models of galaxy formation. I will present new results on the baryonic Tully-Fisher relation (BTFR), which links the total baryonic mass of a galaxy to its outer rotation velocity. I will discuss both successes and failures of LCDM models that attempt to reproduce the BTFR using gas outflows from stellar feedback. ...

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• http://www.mso.anu.edu.au/seminars/abstracts/20141120-1100.html
• Proposed Facility
• Raquel Salmeron - Research Interests and Experience

Decomposition of Galaxy Images and Galaxy Rotation Curves Mosenkov A.V.*^, Savchenko S.S.*, Sotnikova N.Ya.* ... The DECA (DEComposition Analysis) code is designed to investigate images of galaxies in an automatic regime (using the simple 'bulge+disc' model) as well as in manual mode for more detailed images and/or for multicomponent structures. ... The GRCF package was created for performing the galaxies rotation curve decomposition using the models of the bulge, the disc, and the dark halo. ...

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• RADIOSUN Workshop 2014
• The XIII Russian-Finnish Symposium on Radio Astronomy
• Pulkovo EOP and Reference Systems Analysis Center (PERSAC)

... Authors: Spyros Basilakos (Imperial College London) . ... Title: Populating a cluster of galaxies - I. Results at z=0 . ... Title: The Merger Rate to Redshift One from Kinematic Pairs: Caltech Faint Galaxy Redshift Survey XI . ... Title: Multi-wavelength observations of an evolved galaxy group: An endpoint of galaxy merging? ... 23 matches for the search pattern galaxy merging . The URL for this page is: http://xxx.itep.ru/find/astro-ph/1/galaxy+merging/0/1/0/past,all/0/0 www-admin@xxx.lanl.gov ...

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• Description of SED models
• astro-ph authors/title/abstract search for 'galaxy cluster' (skipped 200) all
• "Radio galaxies and cosmology"

... Galaxy Evolution home . ... Regulating the ISM and star formation . Cosmological evolution of star-forming galaxies . The origin and evolution of radio sources . Radio sources and their environments . ... Observations of the local Universe clearly demonstrate that very active star formation phases (starbursts) are often associated with interacting and merging galaxies and that in these systems much of the short wavelength emission is absorbed by dust and re-emitted in the IR. ...

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• Paper II: Spinning dust in galaxies Bojan Nikolic web pages (r. 329)
• Paper I: Method Bojan Nikolic web pages (r. 329)
• Galaxy Evolution: The origin and evoltuion of radio sources

Next: DIRECT MASSES FOR BXCIR Up: EXTREME HELIUM STARS: PULSATION Previous: PULSATION PROPERTIES . As already indicated, V652Her is an important EHe star because its relatively short pulsation period and large amplitude pulsations allow its overall dimensions to be determined with high precision. ... Saio & Nomoto (1998) made the first successful models for the merger of two carbon-oxygen white dwarfs, and prompted Saio & Jeffery (2000) to attempt models for the merger of two helium white dwarfs. ...

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• EVOLUTION MODELS
• Armagh Observatory
• STELLAR PROPERTIES

Find Similar Abstracts . ... ASTRONOMICAL MODELS, GALAXIES, TOPOLOGY, UNIVERSE, ADIABATIC CONDITIONS, CELLS, GALACTIC CLUSTERS, SPATIAL DISTRIBUTION . ... The topological structure of the universe on a scale of a few to 100 Mpc is examined, reviewing the results of recent theoretical investigations. ... Use: Authors Title Abstract Text Text Query with Keywords Return: Query Results Query Form Database: Astronomy Instrumentation Physics and Geophysics ABSTRACT QUERY USER FEEDBACK HELP ...

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• The Model
• Model of the Galaxy
• Evolution of the double neutron star merging rate and the cosmological origin

... Dark Matter Ring Modeled around Galaxy Cluster CL0024 17 . ... A new observation of gravitationally magnified faint galaxies far in the distance behind a massive cluster of galaxies is shedding new dark on the subject. ... A hypothesis for the formation of the huge dark matter ring holds that it is a transient feature formed when galaxy cluster CL0024+17 collided with another cluster of galaxies about one billion years ago, leaving a ring similar to when a rock is thrown in a pond. ...

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• Астронет > Dark Matter Ring Modeled around Galaxy Cluster CL0024 17
• Астронет > Archive of Astronomical and Astrophysical Transactions
• Journal "Peremennye Zvezdy"

Russian SHAREABLE DATA CENTER Institute of Solar-Terrestial Physics SB RAS . ... Although their determination is based on the scattering process model, independent check-ups by rocket experiments have shown their correctness in experimental applications. ... Ionospheric data analysis, especially during strong disturbances, cannot be without some other kinds of diagnostic tools. ... The lack of data has always been a challange in this case. ...

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