... In Figures 2 and 3 we show the 6m telescope spectra of blue compact galaxies HS 1013+3809 and HS 1442+4250, in which typical high excitation HII-region narrow emission lines are seen. ... for red part of HS 1442+4250. ... This correction = 354 km s -1 was calculated for HS 1013+3809 and = 202 km s -1 for HS 1442+4250. ... While HS 1013+3809 looks very symmetric and very compact, with intense star formation burst taking place in its very center, HS 1442+4250 is well elongated, resembling edge-on disk...

Еще в разделе: (Показать все результаты (>2309) - www.sao.ru/ )

• Results and conclusions
• Results of observations
• The Hamburg/SAO Survey for Emission-Line Galaxies

2.5Г-1021 cm-2) have associated dust emission. ... We estimate dust masses of ~104-106 Msolar for the M81 dwarf galaxies, resulting in an average dust-to-gas ratio (Mdust/MHI) of ~3Г-10-4 (1.5Г-10-3 if only the H I that is associated with dust emission is considered); this is an order of magnitude lower than the typical value derived for the SINGS spirals. ... However, the average 70/160 О?m ratio in the sample dwarf galaxies is higher than what is found in the other galaxies of the SINGS sample. ...

Еще в разделе: (Показать все результаты (>18293) - www.stsci.edu/ )

• Practical Validation of Results
• Herschel Images and Results for the Magellanic Clouds
• Science Aided by Deconvolution

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 (>5769) - www.naic.edu/ )

• New Results Confirm Dark Galaxy Existence
• Carl Heiles Conference
• The Arecibo Zone of Avoidance Survey (ALFAZOA)

K-band Arcetri Obscured Supernova Search . What is the KAOSS Project? W hat is the KAOSS Project? Some recent surveys aimed at detecting Supernovae (SNe) in the optical have found that starburst galaxies do not show evidence for an enhanced SN rate, with respect to quiescent galaxies (Richmond et al. ... A similar result was obtained by Navasardyan et al. (2001) who looked for SNe in interacting galaxies, finding no evidence for correlations between SN rate and galaxy properties. ...

Еще в разделе: (Показать все результаты (>7467) - www.arcetri.astro.it/ )

• A local window on galaxy formation with ALMA
• Ionized outflows in z~2.4 quasar host galaxies
• Galaxy archaeology over the last 7 billion years

... 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 (>1474) - mavr.sao.ru/ )

• Galaxy sector, archive 2012
• Galaxy sector, archive 2013
• Galaxy scientific results 2003

M1 image More About M1 Nice Color Picture . ... M16 image More About M16 HST image . ... M31 image More About M31 Nice Color Picture . ... M42 image ; M43 image More About M42/43 Nice Color CCD Picture . M51 image More About M51 Color Image of M51 M51 Supernova . M57 image More About M57 Nice Color CCD Picture Very Deep M57 Image . ... M81 image More About M81 M81 Supernova Ultraviolet Image of M81 More about Ultraviolet Imaging . M82 image More About M82 M82 False Color M82 True Color . ...

Еще в разделе: (Показать все результаты (>484) - zebu.uoregon.edu/ )

• Galaxy Gallery Page IV: The Movies
• Fabry-Perot Images of Ultraluminous Iras Galaxies
• Astronomy Plus CCD Images of Galaxies

... Team . ... The main goal of observations of GRB host galaxies is accumulation of statistics of their spectroscopic and photometric properties. ... The Hubble diagram for 22 GRB host galaxies with known magnitudes and redshifts (GRB 970228, GRB 970508, GRB 970828, GRB 971214, GRB 980613, GRB 980703, GRB 990123, GRB 990510, GRB 990712, GRB 9912008, GRB 991216, GRB 000131, GRB 000210, GRB 000301C, GRB 000418, GRB 000911, GRB 000926, GRB 001109, GRB 010222, GRB 010921, GRB 011121 and GRB011211). ... 600...

Еще в разделе: (Показать все результаты (>1098) - jet.sao.ru/ )

• Search for distant radio galaxies in SAO
• Principal scientific results
• Laboratory for the Stellar Magnetism Study of SAO of the RAS - Home

... By comparison, old elliptical galaxies have a wide range of Lx(gas) and some of them (e.g., group or cluster dominant galaxies) have Lx(gas) 10 or 100 times higher than Lx(LMXB). One of the key observables to address the age effect is the abundance ratio of Fe to elements, b ecause of different pro duction yields of SNe Ia and I I. In the merger scenario of young elliptical galaxies, we would exp ect an enrichment of -elements from SN I I, asso ciated with the recent star formation. ...

Еще в разделе: (Показать все результаты (>3704) - hea-www.harvard.edu/ )

• http://hea-www.harvard.edu/~pgreen/SOC/4.html
• An Example - 3C 120
• Chandra's View of M86

... We present the results of ATCA HI line and 20-cm radio continuum observations of the galaxy Quartet NGC 6845. The HI emission extends over all four galaxies but can only be associated clearly with the two spiral galaxies, NGC 6845A and B, which show signs of strong tidal interaction. We derive a total HI mass of 1.8 x 10 10 Msun, most of which is associated with NGC 6845A, the largest galaxy of the group. ... Figure 2: A new galaxy in the NGC6845 galaxy group. ...

Еще в разделе: (Показать все результаты (>17727) - www.atnf.csiro.au/ )

• The Nature of Boxy/Peanut Spiral Galaxies: Overview and New Results
• Nearby Galaxies
• Normal galaxies in the XMM-Newton fields: X-rays as a star formation indicator

... 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Nuclear activity and environment Effect of environment on AGN is not completely clear yet. ... 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Effect of the mass Mass slices ­ optical and radio AGN overall interaction one-on-one interaction relative location 05/09/2013 Galaxy Evolution over Five Decades - Cambridge 2013 Stratified study Stratifed study that considers several strata of mass. ...

Еще в разделе: (Показать все результаты (>2731) - www.mrao.cam.ac.uk/ )

• The history of star formation and mass assembly in early-type galaxies Bojan
• Understanding Infrared emission from galaxies Bojan Nikolic web pages (r. 329)
• Galaxy Evolution: Regulation of the ISM and Star Formation

... Galaxy Evolution Explorer (GALEX) . ... Searching for SZ clusters . ... Baryon content of galaxy clusters and cosmology . ... 3 sigma peaks: Observational Signatures of High Redshift Galaxies and Low Redshift Clusters . CLUSTERS OF GALAXIES . ... Clusters of galaxies seen in X-rays: war and peace . ... Chandra X-ray Observations of Clusters/Groups/Galaxies . ... Common timing features in neutron stars and black holes . ... X-ray luminosity function of low-mass X-ray binaries in galaxies . ...

Еще в разделе: (Показать все результаты (>805) - hea.iki.rssi.ru/ )

• Fast search through RTT150 data archive
• Zeldovich-100 / International Conference / Moscow, Russia

... 2010 May 29 . Black Holes in Merging Galaxies . ... Explanation: Violent galaxy mergers can feed supermassive black holes. ... New results from a premier sky survey by NASA's Swift satellite at hard (energetic) X-ray energies now solidly show a strong association of AGN with merging galaxies , though. ... In fact, these panels show the location (circled) of Swift X-ray detected supermassive black holes in a variety of merging galaxy systems. ... About APOD | ... A service of: ASD at NASA / GSFC . ...

Еще в разделе: (Показать все результаты (>8299) - www.sai.msu.su/ )

• APOD: July 2, 1995 - The Cartwheel Galaxy
• APOD: 2010 March 30 - Unusual Starburst Galaxy NGC 1313
• APOD: 2006 November 28 - Unusual Starburst Galaxy NGC 1313

... 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 ...

Еще в разделе: (Показать все результаты (>76) - sed.sao.ru/ )

• Informational system "Evolution of RG"
• Methods and results of radio cosmology. Plan.
• "Radio galaxies and cosmology"

Next: NICMOS Coronagraphic Surveys-Preliminary Results Up: No Title Previous: STScI NICMOS Software . NICMOS Coronagraphic Surveys-Preliminary Results . ... Observations with NICMOS . ... The Evolution of Stars seen with ISOCAM - the Need for NICMOS and VLT Follow Up. ... Results . ... The Formation and Evolution of LMC Rich Star Clusters: NGC 1818 . ... HST-NICMOS Observations of Galactic Bulges: Red Nuclei in Nearby Galaxies . ... Investigating the Evolution of Quasar Host Galaxies with NICMOS . ...

Еще в разделе: (Показать все результаты (>242) - www.stecf.org/ )

• The Structure and Composition of High Redshift Radio Galaxies
• NICMOS Imaging of QSO Host Galaxies at 0.1 < z < 4.4
• Limits on the Star Formation Rates of z>2 Damped Ly Systems from H Spectroscopy

... Research . ... A rare hybrid morphology radio galaxy . ... In this project we will be able to investigate the environmental effect on star formation and galaxy evolution in individual galaxies falling into the cluster through radio observations of active galactic nuclei (AGN). Current models of galaxy evolution regulate the star formation rates within the simulated galaxies by invoking radio-mode feedback from AGN. ... Julie.Banfield@anu.edu.au . ...

Еще в разделе: (Показать все результаты (>738) - www.mso.anu.edu.au/ )

• Dark Matter in Spiral Galaxies
• COALA - Computational Astrophysics Laboratory
• CHIAKI's Research

... Director of the RAS ISR . RAS Academician . ... Astrophysics module Kvant of the orbital complex Mir launched in 1987 contains the largest on the station complex of the scientific equipment named the orbital observatory Roentgen. Observatory Roentgen consists of 4 X-ray telescopes, jointly exceeding the range of energies from 2 to 800 keV. ... Among the most significant results that were received in the observatory Roentgen are: . ... measurement of the periods of 9 X-ray pulsars; . ...

Еще в разделе: (Показать все результаты (>181) - www.cosmoworld.ru/ )

... 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 (>1229) - www.cosmos.ru/ )

• Main results of the experimental and theoretical research completed in 2009
• SKA-3 Results Page
• SPACE SCIENCE WEEK

... ESO Science Newsletter May 2014 . ... This newsletter is a summary of recent ESO Science Announcement items. Follow the links or visit ESO Science Announcements to read more. ... Part of the Cycle 2 software is an on-line interface to the ALMA calibrator source catalogue, which will soon be available on the ALMA science portal . ... ESO Workshop, ESO Headquarters, Garching, Germany, 24тАУ28 November 2014 . ... You are receiving this newsletter because you subscribed to the ESO Science Newsletter. ...

Еще в разделе: (Показать все результаты (>66672) - www.eso.org/ )

• ESO - Thesis Topic: ALMACAL: the evolution of the molecular gas in galaxies
• Ultra-compact dwarf galaxies
• ESO - Discs in Galaxies

... The Andromeda Galaxy in Infrared . ... Credit: K. Gordon ( U. Arizona ), JPL-Caltech , NASA Explanation: What is the Andromeda galaxy really like? ... Astronomers trained the orbiting Spitzer Space Telescope at the Messier monster (M31) for over 18 hours, creating a mosaic that incorporated 11,000 separate exposures. ... Publications with keywords: M31 - Spitzer space telescope - infrared . Publications with words: M31 - Spitzer space telescope - infrared . ... Infrared Andromeda . ...

Еще в разделе: (Показать все результаты (>116059) - www.astronet.ru/ )

• Астронет > 3C 295: X-rays From A Giant Galaxy
• Unusual Starburst Galaxy NGC 1313
• The Cartwheel Galaxy

Next: Discussion Up: No Title Previous: Parameters of binary compact . Under the assumptions made above, we can calculate the binary merging rates in the Galaxy R . ... Figure: The dependence of different compact binary merging rates in a model ``elliptical'' galaxy (where all the stars were formed simultaneously at the moment t =0) with mass M . The horizontal line shows the mean merging rate of binary NS in a spiral galaxy of the same mass with a stationary star formation. ...

Еще в разделе: (Показать все результаты (>668) - xray.sai.msu.ru/ )

• Presentation of the results
• ADS Abstract Service Results
• Concluding Remarks and Future Prospects