... The Colorful Clouds of Rho Ophiuchi . ... Characteristic of star forming regions, the telltale red emission from hydrogen gas also permeates the view along with dark, obscuring dust clouds seen in silhouette against the background stars and brighter nebulosities. ... Publications with keywords: Rho Ophiuchi - emission nebula - dark nebula - reflection nebula . Publications with words: Rho Ophiuchi - emission nebula - dark nebula - reflection nebula . ... IC 1396: Emission Nebula in Cepheus . ...

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• The Lagoon Nebula in Three Colors
• Астронет > The Lagoon Nebula in Three Colors
• Астронет > The Colorful Clouds of Rho Ophiuchi

In this gallery are many images of Low Surface Brightness Galaxies which have recently been discovered and analyzed. ... The central surface brightness of this galaxy is 24.28 . Malin 2 This galaxy is another huge disk galaxy with a scale length of 15 kpc and a redshift of 15000 km/a. The high surface brightness knot in one of its spiral arms actually has the same color, luminosity and H-alpha equivalent width as the entire Large Magellanic Cloud . ... Truly it is a Low Surface Brightness Galaxy. ...

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... 2006 July 14 . The Colorful Clouds of Rho Ophiuchi . ... Explanation: This stunning mosiac of the sky around bright stars Antares (Alpha Scorpii ) and Rho Ophiuchi reveals spectacular colors in a cosmic starscape. ... About 500 light-years away, the Rho Ophiuchi star clouds , are well in front of the nearby globular star cluster M4 , visible just below and right of center. ... About APOD | ... NASA Web Site Statements, Warnings, and Disclaimers . NASA Official: Jay Norris. ...

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• APOD: 2002 October 6 - The Lagoon Nebula in Three Colors
• APOD: 2001 August 20 - The Lagoon Nebula in Three Colors
• APOD: 2004 July 23 - Saturns Rings in Natural Color

. (artistic credits: J. English and B. Koribalski) . bkoribal @ atnf.csiro.au

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• Bright prospects: Comparing the H Survey with large-scale radio continuum
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• A Search for Bright Kuiper Belt Objects

Presented on Tuesday, January 7, 2003 . We construct a detailed longitude-velocity diagram through the actual midplane of the Galactic H I disk. The Galactic midplane definition is based on single-dish sky surveys, and the detailed l-v slice ( Fig. 1 ) is extracted from the Canadian Galactic Plane Survey ( CGPS ; Taylor et al. 2003 ). ... Note: other slices offset from this one were not shown in the AAS poster for lack of space, but they are available here . ...

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• M42 Color Images
• HISA Poster for the 33rd Annual Meeting of CASCA, May, 2002
• I-GALFA Reveals Dynamic Events in Our Galaxy

... Подвесные игрушки . ... Тип товара на Маркете: Бриджи детские . ... Тип товара: Бриджи . ... Тип уборки: сухая/влажная . ... Тип пылесборника: мешок . ... Тип пылесоса: обычный . ... Тип: шлифовальная ; . ... Тип установки: врезная; Цвет: светло-серый; Материал: искусственный гранит . ... Тип застежки: молния . ... Тип сумки: для ноутбука . ... Тип товара: Кофты . ...

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Subject, Object and Problems of Astrophysics. Practical and Theoretical Astrophysics. ... Visual Telescope; Problems Which Are Solved with the Its Help. ... Resolution of Telescopes. ... Effectiveness of Telescope in Respect of Resolution. ... Optical Power of Telescopes for Star-like and Extensive Objects. Boundary Magnitude. Reasons of Light Dissipation in Telescopes. ... Spectral Instruments in Astrophysics. ... Basic Photometrical Ideas, Magnitudes and Their Measurement. ...

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• General Astrophysics
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• Gas and dust shells of the Hale-Bopp comet

... Archives . ... Differential Emission Measure [Eqn] . ... Astro 301, class 1, and it took all of 20 minutes of talk about stellar magnitudes to put that notion to permanent rest. ... Now, it turns out that the human eye perceives brightness on a log scale, so magnitudes are numerically similar to log (brightness). ... frac{5}{2}\log_{10}\left(\frac{f_{object}}{f_{standard}}\right) \,,$$ . ... frac{5}{2}\log_{10}\left(\frac{L_{object}}{4 \pi d^2}\frac{1}{f_{standard}}\right) \,.$ ... Chandra Blog . ...

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• Chandra Images for SNR J0505.8-6801
• Chandra Images for 0506-68.0
• Chandra Images for J0454.4-6713

We investigate the dust associated with the supernova remnant (SNR) N49 in the Large Magellanic Cloud (LMC) as observed with the Herschel Space Observatory. N49 is unusually bright because of an interaction with a molecular cloud along its eastern edge. We have used PACS and SPIRE to measure the far IR flux densities of the entire SNR and of a bright region on the eastern edge of the SNR where the SNR shock is encountering the molecular cloud. ... ADS Citation Query . citations = 21 . ...

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• Metallicity Effects on Mid-Infrared Colors and the 8 ЮМm PAH Emission in
• COS Instrument Handbook
• Surface Brightness

... MATERIAL: astronomical data visualization software like ds9 , IRAF, and the two galaxy images in the V-band and I-band . ... You received images in the V and I-band of an unknown, partially resolved Milky Way dwarf satellite galaxy. Your task is to generate a color-magnitude diagram (CMD) of this stellar system, find out what kind of stellar population it is made of (old, young?) and estimate its distance from the sun using well-known features identified in the CMD. ...

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• C/2006 P1 (McNaught)
• RSAA website - Intranet - ANU

Astronomers usually measure the flux of an object by collecting light with a telescope, sending it through a known filter, and then determining the power. ... But astronomers usually give their photometric results in terms of magnitudes. ... Astronomers define an absolute magnitude that is independent of the distance of a star and only depends on the intrinsic properties of the object: the absolute magnitude is the magnitude the star would have if it were 10 parsecs away from the Earth. ...

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• "Structure" publications in 2004 year
• The ROSAT All-Sky Survey Bright Source Catalogue
• Balloon Model in Java

... I. Mean Surface Brightnesses and Integral Color Indices for Bars Gusev A.S. ================================================================================ Abstract: UBVRIJHK surface brightnesses and color indices of bars of galaxies are determined using surface photometry data for 100 barred galaxies (table1.dat). ... J0 Mean surface J0 brightness 46 A1 --- CI- CI sign 47 -50 F1.2 magn/sq.arcsec. U-B)0 (U-B)0 color index 52 -55 F1.2 magn/sq.arcsec. ...

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• http://lnfm1.sai.msu.ru/~rastor/Ralf_Bender/imprs_chapter_11_2007_dwarf_galaxies.pdf

Left: An image in the near infrared (1.65 ЮМm) around RY Tauri, using a special mode of the Subaru HiCIAO coronagraph, the polarized intensity image. This type of observation is preferred for faint emissions associated with scattered light around planet-forming disks, as there is less light from the much brighter star. ... A white ellipse shows the position of the midplane of the disk, which is observed at millimeter wavelengths. ... Right: Schematic view of the observed infrared light. ...

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• http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BD73D972F-C62F-46C4-9B3D-2778DED93D8F%7D
• Dawnт??s Ceres color map reveals surface diversity | Astronomy.com
• Why do some stars appear to flash a variety of different colors when you look

... Click here to go directly to the Orion Nebula Images. ... Copies of individual figures from this paper are available from John Bally . ... Figure 1: The core of the Trapezium showing the four energetic massive stars and a plethora of Sun-like stars with surrounding extended emission. ... Click to download figure in jpeg format. Click to download figure in tiff format. ... Figure 3: A gallery of star-disk systems in Orion's Trapezium. ... To Doug Johnstone's Scientific Home Page . ...

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• APOD: August 6, 1998 - Infrared Horsehead
• Ida - Galileo
• APOD: May 22, 1996 - Star Cluster in the Rosette Nebula

Supernova 2002fk in NGC 1309 . This page is devoted to information on Supernova 2002fk in NGC 1309 Basic information on this SN, including the last reported brightness, on this Supernova can be found on the main page . Information on the original web pages for many of these images can be found on the updates and links web pages. ... 2002/09/19.848 . ... JM Llapasset image . ... 13.0 . ... Josep M. Bosch . ... Josep M. Bosch image . ... vsnet-campaign-sn 476 ] SN 2002fk in NGC 1309 . ...

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• Bright Supernova Bright Supernova
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... V838 Mon is a member of a new class of eruptive variables which appear as a peculiar novae having late K-M type spectra in their outburst. Before its outburst, it was a wide binary system of B3V type stars. ... The B3V companion was seen in the outburst in the UV spectrum taken with HST (Rauch et al., ... In the latest spectra, the light of B3V companion was predominating in the short-wave photometric bands. ... CCD blue frames of V838 Mon before the eclipse (left) and in the eclipse (right). ...

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• http://jet.sao.ru/jet/~goray/comet17p/17p.htm
• Laboratory of radio astrophysics
• how-to.ru : Русская документация : Vim Color Edi/tor HOW-TO (Vi Улучшенный с

... The department was founded in late sixties by Prof. D.Ya.Martynov, who for many years was also the director of Sternberg Astronomical Institute. At present time, the head of the department is Prof. A.M.Cherepashchuk, a pupil of D.Ya.Martynov and his successor as the director of SAI. Since Prof. Martynov, the scientific activity of the department was primarily related to binary stars. ... The department consists of 15 members most of which have Ph.D. in Astrophysics. ...

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... 11 Yellow-Green (78% transmission): Contrasts well with the red and blue characteristics of surface features on Jupiter and Saturn. ... 82A Light Blue (73% transmission): Useful on the Moon, Mars, Jupiter, and Saturn, this subtle pale blue filter enhances areas of low contrast while avoiding significant reduction of overall image brightness. ... Meade Series 4000 Photo-Visual Color Filters may be ordered individually or in the following sets: . ... Meade Series 4000 Broadband Nebular Filters . ...

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Imaging photometry of the optical continuum during Deep Impact Tanyu Bonev1 and Klaus Jockers Max Planck Institute fЭr Aeronomie · Feasibility · Brightness and color measurements of a disintegrated comet · Simulations of the impact ejecta dust cloud · Conclusions 1 on leave from I nsti tute of Astronomi e, Bulgari an Aca demy of Sc i ence s Feasibility or · What we know about the dust coma of comet 9P/Tempel? and · Is the material added by the impact sufficient to be detected? ...

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• The hidden fires of the Flame Nebula* | ESO
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... SEARCH ASP SITE: Match ALL words Match ANY word . ... ASP Conference Series . ... Accidental Astrophysics: The Devil's In the Magnitudes, Part II . ... The star second to the Sun in brilliance is Sirius. ... Recall the magnitude system, passed down to us through a hundred generations of sky watchers, as a means of quantifying stellar brightness ("Accidental Astrophysics," May/June, p. 9). ... Yes, it is a magnitude difference, but that difference is due to the distance between us and the star. ...

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• ASP: Star Science in the Autumn Sky
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