Welcome to the Starburst and Galaxy Evolution website.

Еще в разделе: (Показать все результаты (>12081) - www.stsci.edu/ )

• Starburst and Galaxy Evolution Introduction
• Starburst and Galaxy Evolution
• Links to Models External to STScI

Chiaki Kobayashi, Ralph Sutherland How galaxies did form and evolution? - to answer this unsolved problem, we are simulating the formation and evolutionary history of galaxies in the Universe, including star formation, supernovae feedback, and chemical enrichment. Comparing the spacial distribution of elements within galaxies with observations, we will examine fundamental physical processes that drive galaxy formation. ... COALA : Universe Galaxy AGN Star Planet ...

Еще в разделе: (Показать все результаты (>647) - www.mso.anu.edu.au/ )

• Towards a Truly Unified Model of AGN
• Giant Galaxy String Defies Models of How Universe Evolved
• RSAA Honours Courses (2006)

The project of the informational system creation on the problem of evolution of radio galaxies, as a part of the "Big Trio" project aimed on studing of distant radio galaxies, is designed. This system allows a user to operate with simulated curves of spectral energy distributions (SED) to estimate ages and redshifts by photometry data. Authors use SEDs of several models for different types of galaxies. ... The HTTP and e-mail access is organized to this system. ...

Еще в разделе: (Показать все результаты (>60) - sed.sao.ru/ )

• Description of SED models
• Radio galaxies
• astro-ph authors/title/abstract search for 'galaxy merging' all years

... 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. ...

Еще в разделе: (Показать все результаты (>3238) - www.mrao.cam.ac.uk/ )

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

... As a summary I present a probable model for the evolution of the nearby starburst galaxies by taking into account observations of their large-scale and nuclear gas dynamics as well as numerical simulations of gas flows in galaxies. ... Thus, it is very likely that galaxy interaction plays an important role in the formation of bars . ... A good example is the barred starburst galaxy NGC 1808. ... In fact, one can nearly see the gas flowing toward the galaxy centre where it fuels the nuclear starburst...

Еще в разделе: (Показать все результаты (>7522) - www.atnf.csiro.au/ )

• ATNF Daily Astronomy Picture
• WALLABY - the ASKAP HI All-Sky Survey
• Towards a Truly Unified Model of AGN: Aspect, Accretion and Evolution

... 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 ] . ...

Еще в разделе: (Показать все результаты (>7749) - www.arcetri.astro.it/ )

• Tracing Dust in Spiral Galaxies
• research field
• Clumpy dust disks

... A model for the chemical evolution of a disk galaxy is presented. The model reproduces all the basic . ... investigations of the star formation history. ... the galaxyЫand incorporating a delay in the onset of star formation make it possible to model different scenar- . ios for the evolution of a galaxy's luminosity. ... evolution of massive galaxies. ... of reconstructing the star-formation history and galactic luminosity from observations of galaxies at different . ...

Еще в разделе: (Показать все результаты (>49) - www.inasan.rssi.ru/ )

• Publications of Dmitri Wiebe
• Future of the Galaxy
• Gradients in Disk Galaxies

.

Еще в разделе: (Показать все результаты (>91) - comet.sai.msu.ru/ )

• Previous and Proposed

. First page Back Continue Last page Overview Graphics .

Еще в разделе: (Показать все результаты (>2715) - www.naic.edu/ )

• The Evolution of Galaxies through the Neutral Hydrogen Window The Evolution of
• The Evolution of Galaxies Seen Through The Neutral Hydrogen Line The Evolution
• Heiles Symposium Presentations

... Massive stars, having 10-150 masses of the Sun, with metallicities Z tens to hundreds times less than that of the Sun (Zo), are the main regulators of the galaxy formation and evolution processes in the early Universe. ... In this galaxy, using the 6 m BTA telescope, a new massive blue variable star with high luminosity (>=10 5 Sun's luminocities in visible light) was found. As far as its properties are concerned, this star falls into an LBV (Luminous Blue Variable) class of stars. ...

Еще в разделе: (Показать все результаты (>1336) - mavr.sao.ru/ )

• Lack of Dwarf Galaxies in the Local Volume Compared to Conventional Cosmology
• Measurement of the dark halo shape in polar ring galaxies
• Galaxy sector, archive 2012

Next: Initial binary parameters Up: Population synthesis of Previous: Introduction . Monte-Carlo method for statistical simulation of binary evolution was originally proposed by Kornilov & Lipunov (1983a,b) for massive binaries and developed later by Lipunov & Postnov (1987) for low-massive binaries. ... Recently Leitherer & Heckman (1995) have modelled star formation for elliptical and spiral galaxies, taking into consideration only the single stars. ... Initial binary parameters . ...

Еще в разделе: (Показать все результаты (>638) - xray.sai.msu.ru/ )

• Effect of sources evolution on
• Evolution of the double neutron star merging rate and the cosmological origin
• Conclusions

... The search for distant objects which can be both galaxies and quasars is one of the most important problems of observational astrphysics, because it allows one to determine cosmological parameters connected with the time of appearence and evolution of stellar systems, large scale structure of the Universe. ... Radio galaxies are important objects to be studied because they are sources of infrared-optical-ultraviolet continuum, emission lines and continual radio emission. ...

Еще в разделе: (Показать все результаты (>1264) - jet.sao.ru/ )

• Papers of Vortex project
• GRB follow-up team

... Dark Matter Ring Modeled around Galaxy Cluster CL0024 17 . ... These are multiple images of a few distant galaxies, showing that the cluster is a strong gravitational lens . ... 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. ... Abell 2218: A Galaxy Cluster Lens . ...

Еще в разделе: (Показать все результаты (>110801) - www.astronet.ru/ )

• Астронет > Dark Matter Ring Modeled around Galaxy Cluster CL0024 17
• Астронет > Archive of Astronomical and Astrophysical Transactions
• Illusion and Evolution in Galaxy Cluster Abell 2667

. 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

Еще в разделе: (Показать все результаты (>390) - www.astro.spbu.ru/ )

• Modelling the Milky Way in the Era of Gaia - JD5 Rationale
• List of publications
• Model of clusters

... WORKSHOP "STELLAR ATMOSPHERES" . THE CHEMICAL AND DYNAMIC EVOLUTION OF STARS AND GALAXIES" . ... Chernomorka , Odessa , Ukraine . ... Modeling and interpretation of the stellar spectra of the usual and peculiar stars. Elemental abundances in the stars of different types and populations of the Galaxy. Chemical evolution of the stars and galaxies. ... Andrievsky S.M. (OAO ONU, Odessa, Ukraine) . ... CHEMICAL and DYNAMIC EVOLUTION STARS and GALAXIES" . ... Odessa mailto:astro@paco.odessa.ua . ...

Еще в разделе: (Показать все результаты (>74) - sai.msu.ru/ )

... 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? ...

Еще в разделе: (Показать все результаты (>426) - zebu.uoregon.edu/ )

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

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: Dynamical models of multiple globular cluster populations around massive galaxies . ... Different techniques have been devised to separate multiple GC populations and perform dynamical analyses. ... Within this project, the PhD candidate will examine mock models of multiple GC populations around massive galaxies, devising `blinded' functional tests and comparing the possible sources of bias in different techniques....

Еще в разделе: (Показать все результаты (>65951) - www.eso.org/ )

• Publications, Paul Bristow
• ESO - PhD Thesis Topics offered by ESO Faculty Members
• Model of the evolution of the material around the old star R Sculptoris over

home education > activities . ... Quick math activity that asks students to calculate scale models of a binary star system with a black hole in it. [h] . ... Students use a radiometer and a light bulb with a dimmer switch to make connections between the temperature, color, and radiation output of a star. ... This demonstration, similar to the above, from the Exploratorium Snack-book of science activities, lets students demonstrate how molecules scatter light and change the colors of the beam. [m,h] . ...

Еще в разделе: (Показать все результаты (>842) - www.astrosociety.org/ )

• ASP: The Universe At Your Fingertips Activities TOC
• ASP: Astronomical Society of the Pacific Presents Pricilla and Bart Bok Awards
• ASP: Sharing the Universe

Next: MASSES Up: EXTREME HELIUM STARS: PULSATION Previous: STELLAR PROPERTIES . ... Following main-sequence evolution, a red giant star in a close binary system may expand to fill its Roche lobe. ... Although Iben & Tutukov (1984) used this model to account for the EHes, the latter are not binaries (Jeffery et al. ... Final helium-shell flash in a post-AGB star. ... Accretion from the disk onto the surviving WD creates a star with a degenerate CO core and a helium envelope. ... Other models. ...

Еще в разделе: (Показать все результаты (>1941) - star.arm.ac.uk/ )

• Armagh Observatory
• Stars Beyond Maturity
• W.M. Napier, Senior Research Fellow

... Tonight's Sky . ... The Magazine . News . Observing . ... Community . ... Magazine . ... Gravitational wave search provides insights into galaxy evolution and mergers . ... The double star 54 Leonis, spiral galaxy NGC 3198, and emission nebula NGC 3199 . ... Open cluster NGC 2818, spiral galaxy NGC 2964, and spiral galaxy NGC 2976 . ... Astronomy for Kids . ... galaxy evolution . ... Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter. ...

Еще в разделе: (Показать все результаты (>6657) - www.astronomy.com/ )

• Inside the cyclic model of the universe | Astronomy.com
• Cosmic evolution in a computer | Astronomy.com
• Hubble observes galaxies' evolution in slow motion | Astronomy.com