Rastorguev А.S. "Astronomical Distances" (Lecture course for postgraduates, 2009-2016) . Part 1. ... Trigonometric parallaxes of stars. Moving clusters distances. ... Photometric distances: general approach. Normal stars as "standard candles". ... Main Sequence fitting or distance scale of star clusters. ... Moving photospheres technique. Cepheid distance scale and P-L relations. RR Lyrae distance scale. ... Globular clusters luminosity function. ...

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• Maidanak Lab page

. Supernova Remnants . Image of supernova remnant E0102-72.3 Located in the Small Magellanic Cloud galaxy 190,000 light years from Earth. Image of the Crab Nebula: Supernova Remnant. The supernova was observed by the Chinese in 1054 AD was visible in the daytime for 23 days and 658 days total by the naked eye until it faded from sight. Part of the Vela Supernova Remnant . (**The green line is the trail left by a satellite.) . Full image of the Vela Supernova Remnant . Student Home . Picture Home .

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• http://hea-www.harvard.edu/CHAMP/EDUCATION/PUBLIC/whitedwarfs_pics.html
• The AstroStat Slog Blog Archive Quote of the Week, Aug 23, 2007
• The AstroStat Slog spatial statistics

... Pulkovo Observatory Collection consists of astronomic photographic negatives (plates) dated from 1893. ... Pulkovo Normal Astrograph (plate size 160x160 mm. , scale 59''.56 in mm.) under observational programs: minor planets, major planets, globular and open star clusters, planetary nebulas, selected areas with galaxies, double and multiple stars, bright stars, nova and supernova, comets, Selected Areas, Catalogue of Geodetical Stars (CGS), Photographic Catalog Faint Stars(FCFS) . ...

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... Australia Telescope Compact Array . ... Compact Stellar Systems in the Fornax Cluster: Super-massive Star Clusters or Extremely Compact Dwarf Galaxies? ... We suggest that these objects are either super-massive star clusters (intra-cluster globular clusters or tidally stripped nuclei of dwarf galaxies) or a new type of low-luminosity compact elliptical dwarf (``M32-type'') galaxy. ... Keywords: galaxies: star clusters -- galaxies: dwarf -- galaxies: formation . ... Properties of the compact objects ...

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• Stellar Evolution Links
• Radio Images of the Globular Cluster 47 Tucanae
• RV Tau Variables in Globular Clusters - clues on their nature?

N NGC N Созв. ... C-1 NGC 188 Cep OC Open cluster 00h 44.4m +85 20' 8.1 14 C-2 NGC 40 Cep PN Planetary nebula 00h 13.0m +72 32' 12.4 0.6 C-3 NGC 4236 Dra SG Spiral galaxy 12h 16.7m +69 28' 9.7 19 x 7 C-4 NGC 7023 Cep BN Bright nebula 21h 01.8m +68 12' -- 18 x 18 Refl. nebula C-5 IC 342 Cam SG Spiral galaxy 03h 46.8m +68 06' 9.2 18 x 17 C-6 NGC 6543 Dra PN Planetary nebula 17h 58.6m +66 38' 8.1 5.8 Cat's Eye Neb. ... C-103 NGC 2070 Dor BN Bright nebula 05h 38.7m -69 06' -- 40 x 25 Tarantula Neb. ...

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... The interstar media . The interstar media includes the rarefied substance (gas and dust) electromagnetic radiation, the space beams, neutrino and other kinds of materia which fill the space (see the circulation of gas and dust in the Universe ). ... The nebula of the Alter . ... The gas-dust nebulas. ... The gas nebulas galaxical are shining due to the transformation of the shot waved (ultraviolet) radiation of the very hot stars located in the nebula or near it into the visible light. ...

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• tumor1photoe

Stationary Shock Waves. ... Influence of Medium Ionization on Shock Wave Propagation. Shock Waves with Decays. ... Results of Classic Theory of Radiation of the Electron Moving in Ion Field. ... Classification and Physical Features of Galaxies. X-Radiation of Coronae of Elliptical Galaxies and Clusters of Galaxies. ... Methods of Obtaining of Information about Physical Conditions and Components of Interstellar Medium. ... Ionization Fronts and Shock Waves in the Interstellar Medium. ...

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• Spherical and Practical Astronomy
• Stellar Astronomy

... High Energy Gamma-Ray Astronomy" Symposium | ... ANNOUNCEMENT Dear Colleague, We would like to invite you to participate in the International Symposium on "High Energy Gamma-Ray Astronomy", to be held June 26-30, 2000, in Heidelberg, Germany. The idea of the Symposium is to discuss the basic topics and the objectives of the rapidly developing field of gamma-ray astronomy in the high energy regime above 10 GeV. ... High energy counterparts of Gamma-Ray Bursts. ... Gamma rays from Dark Matter. ...

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• Science with CXO
• ADS Abstract Service Results

STEP INTO THE BLUE - MEADE INSTRUMENTS PRODUCT GUIDE . ... Telescopes . LX850 Series . ... Superb optical performance coupled with time proven computerized pointing and tracking has made the LX200 ACF series a best-seller in the high-performance telescope class. ... Meade's revolutionary LS LightSwitchтДв series of telescopes use advanced technologies to do what no other consumer telescopes have done before: take all the hassle out of using a telescope. ... LightBridge Series . ... Spare Parts . ...

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... NGC 2244 Rosette Cluster - рассеянное скопление Caldwell 50 (C50) у 12 Monocerotis (12 Mon) в созвездии Единорог (Monoceros) .. ... NGC 2244 Rosette Cluster - рассеянное скопление Caldwell 50 (C50) у 12 Monocerotis (12 Mon / open cluster near 12 Monocerotis) в созвездии Единорог (Monoceros (http://www.starlab.ru/showpost.php?p=149205&postcount=1)) .. ... NGC 2244 Rosette Cluster .: . ... Искомый кластер NGC 2244 Rosette Cluster (Collinder 99) будет находиться в 2.5? к югу (S) от 13 Monocerotis .. ...

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• Mayall II (Globular Cluster G1 (G1) / M31 G1) - шаровое звездное скопление в
• Общая Астрономическая Конференция - Показать сообщение отдельно - NGC 2244
• Общая Астрономическая Конференция - Показать сообщение отдельно - Jewel Box -

... Telescope . ... Images . ... Optical pulsations of Crab pulsar (33 ms period). The optical image of Chandra Galactic ultra deep field (1.5-deg field). Mosaic, pseudocolors are from images in g',r',i' . Full screen (JPG, 0.3Mb) . ... The central part of Coma galaxy cluster. Full screen (JPG, 0.6Мб) . ... The optical image of distant galaxy cluster cl0230+1836 (z=0.80) from 400d X-ray cluster survey . ...

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• The best images from RTT150
• Second Spectrum-RG/eROSITA Conference
• SODART_OB_parts

... Future seminars . P a s t seminars . ... The Whisper experiment on-board the Cluster mission: multipoint observations on density and wave structures " . ... In a first part, will by present the instrument: functioning, quantity measured, performances, typical observations. In a second part, will be present wave observations in various regions of the magnetosphere, and indicate a few directions of ongoing studies or considered . ... In a third part, will be discussed density structures. ...

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• ExoMars: Russian part
• Particulas Energeticas
• Movimiento de Particulas Atrapadas Magneticamente -- Historia

... galaxies: bulges galaxies: clusters: general galaxies: clusters: individual: . ... star formation statistics stellar content structure Cosmology ( cosmology :) cosmic background radiation ( cosmology :) cosmological parameters cosmology : miscellaneous cosmology : observations cosmology : theory ( cosmology :) dark ages, reionization, first stars ( cosmology :) dark energy ( cosmology :) dark matter ( cosmology :) diffuse radiation ( cosmology :) distance scale ( cosmology :) early Universe (...

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• Russian part of TORTORA team
• Measurement of the dark halo shape in polar ring galaxies

... Bad Astronomy . ... Bitesize Astronomy . ... Last week , I talked about the inner ring around Supernova 1987A, and a little bit about what we learned about it from early Hubble observations. ... No one knows exactly when the bulk of the supernova debris will hit the ring. ... If the fastest moving debris had finally hit the ring, we'd expect to see more of the ring get hit! ... As the debris hits the ring, it will light up once again, and we will once again see the ring in all its glory. ...

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• Phil Plait's Bad Astronomy: Mad Science
• Phil Plait's Bad Astronomy: Info

... The most powerful and widely used methods to calculate the scattering matrix of a fractal cluster are based on the coupled dipoles methods (e.g. the Discrete Dipole Approximation, DDA) and the theory of light scattering by a cluster of spherical particles [2-4]. ... At present the procedure of calculation of the scattering matrix is well developed for both an oriented cluster of spherical particles and for chaotically oriented clusters of such particles [4]. ...

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IFP gallery SCORPIO (since 2000). Here some data observed on the 6m telescope with IFP installed in the SCORPIO focal reducer are presented. ... Velocity field . Mkn 1157 was observed 1 Sep. 2002 in the Ha emission line. Texp =32x240 sec, seeing 1.5", IFP260. ... This galaxy was observed September, 23 2000 in the Ha emission line, Texp=32x120 sec, seeing 2.5", IFP260. ... PV Cep was observed at the 6m telescope in May, 25 2003 in the [SII] 6716A with IFP501, Texp=36x200 sec, seeing 1.0". ...

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• Results scientific researchs LRS
• Results scientific researchs 3
• References LRS

... Correia, S., Carbillet, M., Fini, L., Bertero, M., Boccacci, P., Vallenari, A., Richichi, A., & Barbati, M. 2001, in ASP Conf. ... AIRY is a modular software package designed to simulate optical and near-infrared interferometric observations and/or to perform subsequent image restoration/deconvolution. ... Bertero, M., Boccacci, P., Correia, S., & Richichi, A. 2000, in Interferometry in Optical Astronomy , ed. P. J Lena & A. Quirrenbach, SPIE 4006, 514 . ...

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• ADASS 2003 Conference Proceedings
• A Commodity Computing Cluster
• Object Detection Using Multi-Resolution Analysis

GCVS Research Group: . Recent publications . Kazarovets E.V., Samus N.N., Durlevich O.V., Kireeva N.N., Pastukhova E.N., The 81st Name-List of Variable Stars. ... Kazarovets E.V., Samus N.N., Durlevich O.V., Kireeva N.N., Pastukhova E.N., The 80th Name-List of Variable Stars. ... Samus N.N., Kazarovets E.V., Kireeva N.N., Pastukhova E.N., Durlevich O.V. General Catalogue of Variable Stars: Current status and new Name-lists Odessa Astronomical Publications, 2010, V. 23, p. 102-105. ...

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• GCVS Research Group: Homepage.
• Index of /groups/cluster/gcvs/gcvs/nsv
• Index of /groups/cluster/gcvs/gcvs/iii

FSP1 : The time intervals corresponding to the INTERBALL TAIL PROBE (IB_TAIL) or GEOTAIL passage through the simulative magnetosphere boundary layer (BL) . ... FSP3 : That part of the FSP1 or FSP2 time intervals, which corresponds to the magnetic conjugations between any couple of the considered spacecraft. The value of the relative geocentric angular distance between magnetic field line's footprints is considered during FSP3 situation selection. ...

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• Substorm expansion phase [Oulu]
• SOIR (Solar Occultation in the Infra-Red) is a part of the SPICAV/SOIR
• The Origin of the Solar System

... MAO main . ... The DRAGON globular cluster simulations: a million stars, black holes and gravitational waves . ... simulations of globular clusters with a million stars on the high-performance . ... of stars in globular clusters at unprecedented detail but also shed light into . the dark world of black holes. ... clusters of single and binary black holes. ... of a globular cluster. www.mpa-garching.mpg.de/328833/hl201603 . ... MAO/NASU, 27 Akademika Zabolotnoho St. 03680 Kyiv, Ukraine . ...

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• The Laboratory of Astrometry
• MAO NASU :: Topic: [ilrs-sta] Old laser parts to give away (1/1)
• MAO NASU :: Topic: Advances in Asteroid and Space Debris Science and Technology