DAILY REPORT #1674 PERIOD COVERED: 0000Z (UTC) 07/12/96 - 0000Z (UTC) 07/15/96 Daily Status Report as of 197/0000Z 1.0 ACTIVITIES SCHEDULED AND ACCOMPLISHED: 1.1 Completed Five Sets of WF/ PC-2 6253 (Pure Parallel Archive Program) The WF/ PC-2 was used to execute a pure parallel program taking = ultraviolet observations running concurrently with prime science = observations ... The = observations were completed as scheduled, and no problems were reported. ...

Еще в разделе: (Показать все результаты (>26084) - www.stsci.edu/ )

• http://www.stsci.edu/ftp/observing/status_reports/hst_status_02_06_02
• http://www.stsci.edu/ftp/observing/status_reports/hst_status_01_25_02
• http://www.stsci.edu/ftp/observing/status_reports/hst_status_02_15_02

... 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 (>1136) - jet.sao.ru/ )

• RESEARCH PROBLEMS of the LRS

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 (>56) - sed.sao.ru/ )

• Group for study of galaxies and cosmology, history
• Radio galaxies

... Science Activities > PhD Thesis Topics offered by ESO Faculty Members > Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies using ALMA calibrator observations . ... ALMA . ... ESO-MIDAS . ... It is therefore essential to probe the evolution of cold gas over cosmic time. ... We are looking for an enthusiastic PhD student who is interested in working with us in using ALMACAL to address exciting and topical science questions related to the evolution of molecular gas in galaxies. ...

Еще в разделе: (Показать все результаты (>67072) - www.eso.org/ )

• ESO - Studying the Cosmological Evolution of Galaxy Clusters with (Sub-)mm
• ESO - Phase 2 Submission
• ESO - Newsletter July 2014

... 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 ...

Еще в разделе: (Показать все результаты (>4479) - www.mrao.cam.ac.uk/ )

• Galaxy Evolution: Cosmological evolution of star formation
• Galaxy Evolution: Regulation of the ISM and Star Formation
• Galaxy Evolution: The origin and evoltuion of radio sources

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 (>760) - www.mso.anu.edu.au/ )

• Philip Lah's Research
• CHIAKI's Presentations
• CHIAKI's Research

... Structure and evolution of galaxies . The Magellanic Stream and high-velocity clouds . ... DINGO the ASKAP deep H i survey . ... In this scenario, small dark-matter haloes are expected to form first and later merge and accrete onto larger haloes to form more massive galaxies like the Milky Way. ... Our Milky Way is surrounded by a vast population of gas clouds, called high-velocity clouds (HVCs), that are mainly detectable in H i emission. ... Compact high-velocity clouds around the Milky Way . ...

Еще в разделе: (Показать все результаты (>30132) - www.atnf.csiro.au/ )

• Structure and Evolution of Galaxies
• Merging Black Holes in Galaxies: Galaxy Evolution, AGN and Gravitational Waves
• ATNF Daily Astronomy Picture

Arecibo Galaxy Environment Survey (AGES) The precursor run is finally complete. Here are some initial results that illustrate the success of the observing technique and also areas where we had problems. ... The channel range selected was the inner 3696 channels, thus avoiding the increase in noise at the edge of the bandpass. ... Each frame of the movie is an image of the observing region from each individual velocity (or frequency) channel in the datacube. ...

Еще в разделе: (Показать все результаты (>5835) - www.naic.edu/ )

• AGES - the Arecibo Galaxy Environment Survey
• The Evolution of Galaxies through the Neutral Hydrogen Window The Evolution of
• The Evolution of Galaxies Seen Through The Neutral Hydrogen Line The Evolution

... 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 (>490) - zebu.uoregon.edu/ )

• The Galaxy Gallery: Messier Objects
• Astronomy HyperText Book
• Physics 410/510 Observational Cosmology

Search for the youngest galaxies and the problems of galaxy formation . During 2 last years of work on the search for new galaxies in the phase of first star formation (SF) burst there were carried out spectral observations of 39 blue compact galaxies (BCGs) - candidates to the most metal deficient unevolved galaxies. 23 of them indeed have appeared new metal-poor galaxies with the oxygen abundance (O/H) (as an indicator of chemical evolution) less than 1/10 of the solar value. ...

Еще в разделе: (Показать все результаты (>2318) - www.sao.ru/ )

• "Structure" publications in 1996 year
• The very metal-poor local dwarf galaxies
• Introduction

... V.V.Makarov, V.P.Reshetnikov, V.A.Yakovleva . Photometric study of the peculiar galaxy NGC 2685" . ... eds.), Tallinn, 1989, p.19 . ... Press, 1994, p.272-273 . ... A.A.Mullari, V.V.Orlov, St.Petersburg Univ. ... conference, St.Petersburg, 1997, p.168-169 . ... All-Russian Astronomical Conference, Book of Abstracts, . ... in "Astronomy: traditions, present, future", V.V.Orlov, V.P.Reshetnikov, N.Ya.Sotnikova (eds.), St.Petersburg University Press, 2007, p.92-115 (in Russian) . ...

Еще в разделе: (Показать все результаты (>319) - www.astro.spbu.ru/ )

• Vladimir P. Reshetnikov's Home Page
• Galaxy chemical evolution
• Chemical evolution of galaxies: list of publications

... Credit Copyright: W. Keel and R. White ( U. Alabama ), NASA Explanation: How much dust is in spiral galaxies? ... This striking, detailed Hubble Space Telescope image of dust in the outer reaches of a foreground spiral galaxy (left) back lit by an elliptical galaxy offers an elegant approach to providing the answers . ... Publications with keywords: dust - spiral galaxy . Publications with words: dust - spiral galaxy . ... Nearby Spiral Galaxy NGC 4945 . NGC 1309: Spiral Galaxy and Friends . ...

Еще в разделе: (Показать все результаты (>110939) - www.astronet.ru/ )

• Астронет > Dusting Spiral Galaxies
• Journal "Peremennye Zvezdy"
• Illusion and Evolution in Galaxy Cluster Abell 2667

... January 16, 1998 . Dusting Spiral Galaxies . Credit: W. Keel and R. White ( U. Alabama ), NASA . Explanation: How much dust is in spiral galaxies? ... This striking, detailed Hubble Space Telescope image of dust in the outer reaches of a foreground spiral galaxy (left) back lit by an elliptical galaxy offers an elegant approach to providing the answers . As expected, dust lanes in the foreground galaxy seem to be associated with spiral arms. ... About APOD > . ... NASA Technical Rep.: ...

Еще в разделе: (Показать все результаты (>4106) - www.sai.msu.su/ )

• APOD: 2007 March 5 - Illusion and Evolution in Galaxy Cluster Abell 2667
• Bilbio
• APOD: 2013 May 14 - Galaxy Collisions: Simulation vs Observations

TALKS ST EL L E Raffaele Gratton INAF - Osservatorio Astronomico di Padova Stellar abundances and the chemical evolution of stellar systems: the Italian contribution The chemical composition of stellar syst the last few years, exciting results have and efficient spectrographs. ... Once the observations of all clusters will be completed for at least one season, we plan to better describe and model the evolution of the stellar angular momentum from the PMS to the TAMS. ...

Еще в разделе: (Показать все результаты (>7310) - www.arcetri.astro.it/ )

• http://www.arcetri.astro.it/radtran/talks/mpohlen.pdf
• http://www.arcetri.astro.it/igm50/talks_all/grossi.pdf
• A local window on galaxy formation with ALMA

... The study of the Large-scale structure of the Universe and measurements of the Dark Energy equation of state; The exploration of the growth and cosmological evolution of supermassive Black holes in the Universe. ... In course of the all sky survey SRG will discover about 100 000 galaxy clusters and 3 million AGNs. Galaxy clusters are the largest gravitationally bounded objects in the Universe and are best explored through the study of X-ray emission from the hot intergalactic gas. ... 2016 IKI RAN ...

Еще в разделе: (Показать все результаты (>780) - hea.iki.rssi.ru/ )

• z90-program
• Second Spectrum-RG/eROSITA Conference

... Space Research Institute . Main . ... Main results of the experimental and theoretical research completed in 2010 . ... Moon's topography is shown based on LOLA laser altimeter data, white contour shows a permanently shadowed region and a white rhomb indicates LCROSS spacecraft impact location. ... Ultra deep survey of the sky in hard X-rays, performed by INTEGRAL observatory . INTEGRAL observatory has completed the first and the most sensitive survey of the sky in hard X-ray energy band. ...

Еще в разделе: (Показать все результаты (>1107) - www.cosmos.ru/ )

• Main research and development work completed in 2009 and ready for
• Main results of the experimental and theoretical research completed in 2011
• Main results of the experimental and theoretical research completed in 2009

... A radio galaxy is a galaxy that emits an unusually big amount of energy at radio wavelengths. ... Inside of each galaxy with an active nucleus (radio galaxies are among them) there must be a system of a "central machine" responsible for the colossal amount of the emitted energy from radio to gamma ranges. ... Sometimes a radio source in an active galaxy may flare again if the needed conditions appear (a new portion of matter would fall into the furnace of the "central machine"). ...

Еще в разделе: (Показать все результаты (>1404) - mavr.sao.ru/ )

• Galaxy sector, archive 2012
• Lack of Dwarf Galaxies in the Local Volume Compared to Conventional Cosmology
• Galaxy sector, archive 2011

... Dept. for Physics of Stars&Galaxies . ... Using a database view Sloan Digital Sky Survey (SDSS), containing almost a million spectra created 15,000 sample galaxies with active star formation, which is used for various studies and physical state of evolution of galaxies. ... Star clusters of the Galaxy . The project MWSC (Milky Way Star Clusters) directory using 2MASS, which includes nearly 500 million vision to the limit Ks = 15.3, analyzed more than 4,000 cluster-like objects in the galaxy. ...

Еще в разделе: (Показать все результаты (>575) - www.mao.kiev.ua/ )

• Dept. for Physics of Stars&Galaxies
• КАРТОТЕКА ПУБЛ?КАЦ?Й СП?ВРОБ?ТНИК?В ГАО НАН УКРА?НИ
• Activity - Page 3

... Session 1 - Stars, star formation, stellar populations and planets . 9.20 10.00 . ... HST Spectroscopy of the Hottest White Dwarfs . ... Coffee break . ... Lunch break . ... A (long) look at neutron stars with HST . ... Session 2 - Nearby galaxies, bulges, spheroids, galaxy formation . ... New HST/ACS Insights into the Evolution of Star-Forming Dwarf Galaxies with Extreme Properties of Cosmological Relevance . ... Deriving properties of Lyman-break galaxies at z~3-5 using HST/VLT/Spitzer data . ...

Еще в разделе: (Показать все результаты (>256) - www.stecf.org/ )

• NICMOS Science
• Investigating the Evolution of Quasar Host Galaxies with NICMOS
• A Color Analysis of NICMOS Parallel Observations

Next: Supernova Explosions Up: No Title Previous: X-ray Luminosity Evolution . The origin of cosmic rays (CR) (especially of very high energies, >  eV) until now has been one of the unsolved problems in modern astrophysics. It is unclear as yet whether one universal mechanism of relativistic particle formation in our Galaxy operates or not, and if there are several different mechanisms, what is their relative contribution to CR formation. ... compact X-ray stars in binary systems. ...

Еще в разделе: (Показать все результаты (>718) - xray.sai.msu.ru/ )

• X-ray Luminosity Evolution
• Evolution of the double neutron star merging rate and the cosmological origin
• Contents