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 ...

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• COALA - Natsuko Izutani

... Classes . ... Class List . ... casa::SpectralList . ... SpectralList ( uInt nmax) . ... SpectralList (const SpectralElement &in) . ... Convert to and from a Record (see details in SpectralElement ). void casa::SpectralList::insert . ... Insert in sort order in the list. void casa::SpectralList::insert . ... References list_p , and casa::PtrBlock< T >::nelements() . ... const SpectralElement & casa::SpectralList::operator[] . ... PtrBlock < SpectralElement *> casa::SpectralList::list_p [private] . ...

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• Late Stages of Stellar Evolution
• casacore: casa::SpectralFit Class Reference
• Sheltran - Description of the language

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . ... Meade Series 5000 HD-60 4.5mm 6-Element Eyepiece (1.25") . ... Meade Series 5000 4.5mm HD-60 6-Element Eyepiece, #07730 (1.25"). The latest advancement in the Meade Series 5000 eyepiece series offers a large 60 apparent field of view and a flat field of view which is tack sharp right to the edge. ... Meade Series 5000 Pl ssl Eyepieces offer a very wide field-of-view, with pinpoint edge of field sharpness and contrast. ...

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• Meade Series 5000 HD-60 6.5mm 6-Element Eyepiece (1.25")
• Meade Series 5000 HD-60 9mm 6-Element Eyepiece (1.25")
• Meade Series 5000 HD-60 25mm 6-Element Eyepiece (1.25")

... Figure: Massive binary evolutionary track. ... A short glance to this track is sufficient to understand that there are a lot of evolutionary scenario parameters, which affect different stages of the binary evolution. Fortunately, a very limited number of parameters has effect on the compact binary merging rate. ... The most important (and practically unique) parameter changing the galactic binary NS merging rate is the distribution of an additional (kick) velocity imparted to NS at birth. ...

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• The COOC Criterion (Criterion of Observations versus Calculations)
• Effect of sources evolution on
• Evolution of the Double Neutron Star Merging Rate andthe Cosmological Origin of

... Bojan Nikolic web pages (r. 329) . A gallery of interacting galaxies . ... The history of star formation and mass assembly in early-type galaxies . ... Abstract . ... Complete plots of radiospec analysis . Analysis of (radio) spectra . ... Nested Sampling in R & analysis of spectra . ... Paper II: Spinning dust in galaxies . ... The search results are restrict to these pages only . ... Copyright 2005 -- 2016, Bojan Nikolic feedback welcome ...

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• The history of star formation and mass assembly in early-type galaxies Bojan
• MERLIN Observations of the Radio Jets of SS433
• _element struct Reference

Armed with these assumptions, observations, and laws, cosmologists try to build a theory of the development, or evolution, of the universe. ... Over the past 70 years, they have constructed and tested a theory that seems to explain the major properties of the universe: the Big Bang theory. ... This is an important point: The Big Bang theory allows for many different scenarios of the detailed evolution and composition of the universe. ... Because of a theory called nucleosynthesis. ...

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• ASP: An Ancient Universe - Changes in the Solar System
• ASP: Cosmology: The Origin, Evolution & Ultimate Fate of the Universe

Welcome to the Starburst and Galaxy Evolution website.

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• GOODS: The Great Observatories Origins Deep Survey
• CSPICE Routines: SET_C
• WFC3 Instrument Handbook

It is a matter of common knowledge that in processes of genesis and evolution of many solar phenomena participate magnetic fields of sunspots. ... As a basis for formation of the database we take data on magnetic fields, collected by set of observatories during many years of observations. ... Section "Magnetic field data" contains data of magnetic field observation for separate sunspots, presented in standard text format (ASCII). ... Description of structure of these files is presented here . ...

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• Pulkovo NEO Page: Ephemeris Support

... Stellar cinders . Born-again stars . ... Heavyweight Stars . ... What will happen inside the Sun and why? ... These are questions about "stellar evolution", the history of stars as they are transformed by nuclear processes deep inside. ... Most of what we know about stellar evolution comes from computer models of stars. ... We learn about the evolution of high-mass stars from HR diagrams of young galactic open clusters, and the evolution of low-mass metal-poor stars from old globular clusters. ...

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• The Chemical Evolution of FGSge
• ULTRACAM Observations of Subdwarf B Stars
• EVOLUTION MODELS

The Stats of Couples From Pairing Algorithms to Binary Mass-Ratio Distributions Yutong Shan Binary Formation: Theory vs. Observation How do we think most Binaries form? ... 2009) Mass-Ratio Distribution: жpik's Law Observed binary mass-ratio distribution is often `fitted' with a power law: жpik's Law: f(q) ~ q q = Msecondary/Mpri mary жpik's Exponent, Equal-mass favoured Unequal-mass favoured Primary Mass (Mprim) Flat Often stated as a function of Primary Mass q = Msec / Mprim (Raghavan et al. ...

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• Smithsonian Astrophysics Observatory Predoctoral Fellowships, 2004

... Stellar Evolution is driven entirely by the never ending battle between Pressure and Gravity . As imbalances are reached, the star is driven to find a new Energy source. ... Pressure and gravitational forces are equal, the star is stable and its core is sufficiently hot to fuse Hydrogen into Helium More about main sequence stars . ... The luminosity generated by the core fusion of Helium into Carbon is far greater than the shell luminosity associated with the fusion of Hydrogen into Helium. ...

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• Formation of the Elements
• Foundations of the Big Bang

... gtibuild constructs an OGIP-compliant table of Good Time-Intervals (GTI) from a plain text description file. A complex fragmentation of the time-line may be described in terms of good and bad intervals, which may be simple or periodic. ... A periodic interval is a good or bad simple interval repeated through a whole number of periods. ... Having simple bad intervals together with a periodic bad interval in the same description file does not create the possibility of unexpected good time. ...

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• xmmtrack: XMM orbit TRACKing

by I.M. Chertok, V.V. Fomichev, A.A. Gnezdilov, R.V. Gorgutsa, V.V. Grechnev, A.K. Markeev, R.W. Nightingale, and D.E. Sobolev . Fig. 2. Inverted TRACE images at 195 illustrating development of the EUV post-eruption arcade with the well-organized loop, two-ribbon, and spine structures. Note that the exposures have been rescaled to the same peak intensity to show the evolution of the bright elements. The field of view is 220.5 by 182 Mm. Back to paper .

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... CB3 0HA, U.K. The UCDs (Unified Content Descriptors) were first developed in the ESO/CDS data mining project, to describe precisely the contents of the individual fields (columns) of tables available from a data center. ... We present different applications of UCDs: selection of catalogues, based on their content; identification of catalogues having similar fields; automated data conversion allowing direct comparison of data in cross-identifications. ... a definition of the corresponding UCD; . ...

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• See Spike Run... Run, Spike, Run
• Synthetic Images of the Solar Corona from Octree Representation of 3-D Electron
• Modelling Spectro-photometric Characteristics of Eclipsing Binaries

... A file upload element on an HTML form. ... JavaScript 1.1: added type property . ... The HTML INPUT tag, with "file" as the value of the TYPE attribute. For a given form, the JavaScript runtime engine creates appropriate FileUpload objects and puts these objects in the elements array of the corresponding Form object. ... form . ... For all FileUpload objects, the value of the type property is "file" . ... Use the value property to obtain the file name that the user typed into a FileUpload object. ...

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• http://www.arcetri.astro.it/~sait07/stelle.pdf
• Index of /science/chianti/chianti_3.03/elements
• IBIS: Technical Description

As in the last years, the Ephemerides of Minor Planets for 2015 are prepared by the IAA RAS only in the electronic form. ... Orbital elements of all numbered planets have been determined in IAA all over again on the ground of available observations in the catalog of the Minor Planet Center. ... More detailed information on orbital elements used in the present volume of EMP and their accuracy is given in section "Information on new orbital elements". ... a) information on new orbital elements; . ...

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• Keywords_152
• EPHEMERIDIES OF MINOR PLANETS (EMP)
• ENGAMPLE

... 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 . ...

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• Publications of Dmitri Wiebe
• Circular Polarization
• Gradients in Disk Galaxies

Ballistic life-time . ... The orbit inclination to the equatorial plane (black line) and to the ecliptic plane (red line) are shown on the third panel. ... The launch orbital elements value and its evolution during flight is shown on the plot for the time interval (August 3, 1995 - October 16 2000). ... The critical parameter is perigee altitude shown on the first panel. ... This parameter determine the IB_Tail ballistic lifetime up to October 16, 2000. ... Dated 25 May, 2000 . ... INTERBALL mission ...

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• The INTERBALL Auroral PROBE orbital elements collections
• From Stargazers to Starships
• STDA files

... Description . ... The SCORPIO-2 project: . ... The multi-mode spectrograph SCORPIO-2 was developed using the experience of observations at the 6-m telescope BTA with the SCORPIO focal reducer . ... The focal reducer consists of several units ('floors') mounted in the common case in the following order (from the telescope focal plane): . ... The focal reducer is connected with the platform-adapter which used for guiding by offset stars and for illumination the spectrograph by calibration lamps. ...

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• harak_e
• Instrumentation
• Introduction

... Development of Ideas of Structure and Evolution of Stars. Integral Features of Stars, Which Determine Their Structure, Direction and Rate of Evolutuion. ... Connection between Potential and Thermal Energy of Star. ... Structure of a Main Sequence Star. Features of Massive Stars Evolution on the Main Sequence. Internal Structure of the Sun. ... White Dwarfs, Their Features. ... Evolution from the Main Sequence of Massive Stars. ... Evolution of Small Mass Stars till White Dwarfs Sequence. ...

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• Laboratory static Fourier-spectrometer
• Celestial Mechanics
• Spherical and Practical Astronomy