... OCR by H.Andernach 1/96, to be proof-read) This is the first of a series of papers presenting results of a 10-GHz radio continuum survey of the galactic plane region using the 45-m telescope at Nobeyama. ... Weak Nonthermal Sources: A comparison with the Bonn S-GHz survey reveals a number of weak nonthermal sources near the galactic plane. ... For this reason we conducted a survey of the galactic plane region at 10 GHz using the 45-m radio telescope at the Nobeyama Radio Observatory (NRO). ...

Еще в разделе: (Показать все результаты (>227) - www.sao.ru/ )

• The RATAN SNRs Survey
• A 20 cm VLA survey of Abell clusters of galaxies

... About ATNF overview . ... Governance overview . Australia Telescope Steering Committee . ... Parkes radio telescope . ... Visiting Parkes radio telescope . ... Parkes radio telescope webcam . ... Finding the Bivariate Brightness Distribution of galaxies from an H I selected sample . ... A method is presented that will enable the bivariate luminosity/surface brightness distribution of galaxies to be determined from a relatively small H I selected sample. ... PICASSO - an automated galaxy finder . ...

Еще в разделе: (Показать все результаты (>14159) - www.atnf.csiro.au/ )

• PhD Thesis (summary)
• The galaxy IC 2554
• HIPASS Bright Galaxy Catalog

HI Distribution in the Region . of the Supernova Remnant G78.2+2.1 ( 2001 ). ... Based on RATAN-600 21 cm line observations with an angular resolution of 2.4' over a wide range of radial velocities, we analyze the neutral-hydrogen distribution in the region of the supernova remnant (SNR) G78.2+2.1. ... The brightness distribution of H I features at a radial velocity of +10 km/s after an extended background in the region of the Cygnus X radio source and SNR G78.2+2.1 has bee subtracted. ...

Еще в разделе: (Показать все результаты (>1139) - jet.sao.ru/ )

• Results scientific researchs 20
• Spectral energy distribution
• Radio sources identfification

. Please standby and you will be automatically connected to the new location of the unframed Supernova page. Or, click on the link above. If you have questions or problems, please email me at David Bishop dbishop@vhdl.org . Last modified: Mon Aug 27 12:40:15 EDT 2001

Еще в разделе: (Показать все результаты (>923) - www.rochesterastronomy.org/ )

• Supernova 2002fk in NGC 1309
• Supernova 2011ht in UGC 5460
• Bright Supernova - Archives

Sternberg Astronomical Institute, Moscow University, . Moscow, Russia . Supernovae make us brighter .. Search russian astronomical resources . Mirror of International Supernovae Network ( Original site ) . Catalogue of Supernovae Stars . HTTP access to SAI Catalogue of Supernovae Stars . SAI SN Light Curves Online . ... Sternberg Astronomical Institute ( in Russian ) . ... Astronet - Russian Astronomical Network . ... Russian Foundation for Basic Research . ...

Еще в разделе: (Показать все результаты (>6378) - www.sai.msu.su/ )

• APOD: 2007 May 10 - SN 2006GY: Brightest Supernova
• Bright Sn in NGC 3877
• APOD: 2014 January 24 - Bright Supernova in M82

... The main field of my investigations is stellar spectrophotometry. As a result of scientific activity of our group spectrophotometric catalog was created including energy distribution data on 900 stars in the range 3200-7600AA and 250 stars in the range 6000-10800AA (Voloshina et al., Spectrophotometry of Bright Stars, ed. I.N.Glushneva, 1982, Moscow, Nauka, in Russian). ...

Еще в разделе: (Показать все результаты (>18) - uranus.sai.msu.ru/ )

... Archives . ... ArXiv] SVM and galaxy morphological classification, Sept. 10, 2007 . ... On the Metallicity-Color Relations and Bimodal Color Distributions in Extragalactic Globular Cluster Systems by M. Cantiello and J. P. Blakeslee . Many observations on globular cluster systems (GCS) show bimodal distributions in color and metallicity space. ... Based on their simulation study, (V-H) and (V-K) are confirmed to be good colors for revealing unbiased bimodal metallicity distributions in GCS. ...

Еще в разделе: (Показать все результаты (>3319) - hea-www.harvard.edu/ )

• Comments on: tests of fit for the Poisson distribution By: hlee
• The AstroStat Slog Blog Archive tests of fit for the Poisson distribution
• The AstroStat Slog Power

A1652 2002-Feb-01 22:31:07 Technical Page Proposal Type: Regular General Category: Astronomy Observation Category: Extragalactic Total Time Requested: 24 Hours Proposal Title: The Spatial Distribution of LSBs in the Pisces-Perseus Supercluster ABSTRACT: Low Surface Brightness galaxies (LSBs) appear to be the remnants of the lowest density fragments of the initial density perturbation spectrum of the early Universe (Impey and Bothun 1997). ... In fact, such traits have been observed for LSBs. ...

Еще в разделе: (Показать все результаты (>4941) - www.naic.edu/ )

• http://www.naic.edu/vscience/schedule/tpfiles/O'NeiltagA1400tp.ps
• HISA Poster for the 197th Meeting of the AAS, January, 2001
• Slide 8

... SN 2006GY: Brightest Supernova . ... 10.05.2007 . ... In fact, given its estimated distance of 240 million light-years, SN 2006gy was brighter than, and has stayed brighter longer than , any previously seen supernova. The Chandra observations in the lower right panel establish the supernova's x-ray brightness and lend strong evidence to the theory that SN 2006gy was the death explosion of a star well over 100 times as massive as the Sun. ... May 2007 . ... Publications with keywords: supernova . ...

Еще в разделе: (Показать все результаты (>106018) - www.astronet.ru/ )

• SN 1006: Historys Brightest Supernova
• Астронет > SN 2006GY: Brightest Supernova
• Астронет > SN 1006: Historys Brightest Supernova

... The distribution of redshifts among the DXRBS FSRQs identified so far (Figure 3) is quite similar to that of the 1 Jy and S4 samples. ... A more thorough comparison will have to await completion of our survey and the convolution of the redshift distribution with the WGACAT sky coverage. As has already been mentioned by Hook et al. (1996), selecting flat-spectrum sources is an efficient way of finding high-redshift, radio-loud quasars. ...

Еще в разделе: (Показать все результаты (>66123) - www.eso.org/ )

• Bright supernova in the LMC | ESO
• The Brightness of the Night Sky
• NTT Observations of Bright Comet 1995 Q1 (Bradfield) | ESO

... Visible Distribution of Galaxies. ... Features of Elliptical, Lens-Shaped, Spiral and Irregular Galaxies. Galaxies with Bar. ... Distribution of Surface Brightness of Surface and Spiral Galaxies. ... Color Characteristics of Galaxies. ... Methods of Galaxies' Mass Determination. ... Hidden Mass of Spiral Galaxies. ... Features of Dark Matter Distribution in E and SO Galaxies. ... The Whole Number of Galaxies and Their Density by the Results of Observation on the 'Hubble' Space Telescope. ...

Еще в разделе: (Показать все результаты (>99) - space.univ.kiev.ua/ )

• Stellar Astronomy
• Theoretical Astrophysics
• Olexiy V. Agapitov presentations & posters

... Armagh Observatory, College Hill, Armagh BT61 9DG, +44 (0)28 3752 2928 . ... Lower panel: The ME spot map of the star in orthographic projection, showing the disc of the star as it would be seen by an observer on the Earth at the labelled rotation phases (see the text). ... We carried out high-resolution spectroscopy and BV(I)C photometric monitoring of the two fastest late-type rotators in the nearby Pictoris moving group, HD 199143 (F7V) and CDтИТ64 1208 (K7V). ...

Еще в разделе: (Показать все результаты (>2380) - star.arm.ac.uk/ )

• Observations and Data Reduction
• Observations with the Faulkes Telescopes
• Coronal Bright Points: Another Oscillating Environment

... 2006: . ... 1) A study of the solar corona. ... 2) The study of the solar northern polar region. A powerful radio source above the solar North Pole in the region of the polar coronal hole was discovered. ... A transition boundary from brightening to darkening at the wavelength of 3.5cm was found in the emission of the polar coronal hole. These facts are decisive for the choice of the solar cycle model. 3) Polarized radio emission of a high-latitude prominence was registered. ... Archive . ...

Еще в разделе: (Показать все результаты (>345) - mavr.sao.ru/ )

• Solar system scientific results 2003
• Measurement of the dark halo shape in polar ring galaxies
• Galaxy sector, archive 2014

... Empirical and theoretical modeling of 3-D structures in the solar corona is confronted by the tremendous amount of data needed to represent phenomena with a large dynamic range both in size and magnitude, and with a rapid temporal evolution. Octree representation of the 3-D coronal electron distribution offers the right compromise between resolution and size, allowing computation of synthetic images of the solar corona. ... The time interval between images is one day. ...

Еще в разделе: (Показать все результаты (>1719) - www.adass.org/ )

• Simulated AXAF Observations with MARX
• Positive Iterative Deconvolution in Comparison to Richardson-Lucy Like
• Using Massively Parallel Processing of a NLTE Spectrum Synthetic Code and an

The revision of the MASS/DIMM star catalogue N. Shatsky, V. Kornilov March 16, 2008 Abstract The compilation of the (updated) version of the MASS (MASS/DIMM) device target catalogue is described. ... Then the list was cleaned according to following criteria: I. Remove stars too faint for a MASS device. ... Here the color equation of the Sternb erg device was taken: M AS S mag = V mag + 0.45 (B - V ); stars with M AS S mag > 3.2 were removed. ... This was made based on the GCVS4.2 catalogue data. ...

Еще в разделе: (Показать все результаты (>22) - curl.sai.msu.ru/ )

• Index of /pub/mirror/opensuse/distribution/

... In recent years much of my observational research has involved observations with the Giant Metrewave Radio Telescope (GMRT), near Pune, India. ... Deep 610-MHz GMRT observations of the Spitzer extragalactic First Look Survey field -- I. Observations, data analysis and source catalogue , Garn, T.S., Green, D.A., Hales, S.E.G., Riley, J.M., Alexander, P., 2007MNRAS.376.1251G . ... Further GMRT observations of the Lockman Hole at 610 MHz Garn T. S., Green D. A., Riley J. M., Alexander P., 2010BASI.. ...

Еще в разделе: (Показать все результаты (>2765) - www.mrao.cam.ac.uk/ )

• G74.0-8.5
• G120.1+1.4
• Supernova Remnant (SNR) Catalogue or Catalog of Galactic SNRs

The radial distribution of metallicity of star-forming galaxies in a galaxy cluster can inform us about the mass assembly and enrichment history of the galaxy cluster. ... Both galaxy clusters are cool-core clusters at redshift z т?? ... The gas-phase metallicity of star- forming galaxies in MACS1115+01 exhibit anti-correlation with projected distance т??0.15 ТБ 0.08 dex/Mpc, whereas the radial metallicity distribution of RXJ1532+30 is statistically flat (т??0.09 ТБ 0.12 dex/Mpc). ...

Еще в разделе: (Показать все результаты (>599) - www.mso.anu.edu.au/ )

• Emma Kirby - Science
• GSAOI Bulk Motions Science Page
• Siding Spring Survey

This all-sky image, constructed from 2 years of observations by NASA's Fermi Gamma-ray Space Telescope, shows how the sky appears at energies greater than 1 billion electron volts (1 GeV). Brighter colors indicate brighter gamma-ray sources. ... A diffuse glow fills the sky and is brightest along the plane of our galaxy (middle). Discrete gamma-ray sources include pulsars and supernova remnants within our galaxy as well as distant galaxies powered by supermassive black holes. ...

Еще в разделе: (Показать все результаты (>6367) - www.astronomy.com/ )

• Bright new supernova blows up in the Cigar Galaxy (M82) | Astronomy.com
• Top Space Stories of 2015: Deciphering a famous supernova | Astronomy.com
• Closest type Ia supernova in decades solves a cosmic mystery | Astronomy.com

A study of Martian surface characteristics using microwave remote sensing technique at S-L-P bands (6-100 cm wavelengths) is suggested. The method is based on measurements of radar backscattering and brightness temperature variations induced by subsurface temperature, moisture, porosity and surface roughness changes. ... Combine active-passive microwave long-time observations are conducted along the route of the "Martian Orbital Station" . ...

Еще в разделе: (Показать все результаты (>649) - www.iki.rssi.ru/ )

• Dayside aurora [Oulu]
• Complex plasma spectrometer SCA-1
• Pluto and Charon

Radio pulsars strictly periodic signals 14.03.2016 B 10 G;E 10 V / cm 12 10 2 Individual pulses and average profile of pulsar 14.03.2016 3 Average profiles of pulsars 14.03.2016 average energy distribution of pulses by phase of period. ... 14.03.2016 5 2695 Giant pulses (GPs) of pulsar Intensity, a.u. Time, ms Pulses that exceed the average profile over 30 times were called giant pulses. ... 2005) 14.03.2016 8 Individual pulses energy distribution 1937+21. ...

Еще в разделе: (Показать все результаты (>239) - www.astro.spbu.ru/ )

• Linear polarization: wavelength dependence
• Fractal Matter Distribution
• Gravity Theory