... Central IC 1805 . ... Credit: Ken Crawford ( Rancho Del Sol Observatory ) Explanation: Cosmic clouds seem to form fantastic shapes in the central regions of emission nebula IC 1805. Of course, the clouds are sculpted by stellar winds and radiation from massive hot stars in the nebula's newborn star cluster (aka Melotte 15). ... Publications with keywords: emission nebula - star formation . Publications with words: emission nebula - star formation . ... Emission Nebula IC 1396 . ...

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• The Colorful Clouds of Rho Ophiuchi
• Астронет > The Colorful Clouds of Rho Ophiuchi
• Journal "Peremennye Zvezdy"

... March 12, 1996 . The Colorful Clouds of Rho Ophiuchi . ... The blue regions shine primarily by reflected light. Blue light from the star rho Ophiuchi and nearby stars reflects more efficiently off this portion of the nebula than red light. ... The Rho Ophiuchi star clouds , well in front of the globular cluster M4 visible on far lower left, are even more colorful than humans can see - the clouds emits light in every wavelength band from the radio to the gamma-ray. ... About APOD | ...

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• APOD: 2005 July 9 - The Colorful Clouds of Rho Ophiuchi
• APOD: 2013 December 3 - The Colorful Clouds of Rho Ophiuchi
• APOD: 2007 September 3 - The Colorful Clouds of Rho Ophiuchi

... Radiance image in Si iv 1402.8 (top-left, in reversed color table), Doppler velocity image (bottom-left), nonthermal velocity image (bottom-right) and HMI magnetogram (top-right) of region "A". ... The yellow box on the Doppler image outlines the region where anti-parallel flows are seen. ... A cluster of such loops was observed on the solar disk in active region NOAA11934, in the Si iv 1402.8 spectral raster and 1400 slit-jaw (SJ) images. ...

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... Values have been scaled arbitrarily. High ratios are shown in blue, corresponding to blue colors, and low ratios are shown in red, corresponding to red colors. ... Noise combined with background subtraction difficulties in the lower left quadrant of the WISP1 data (see Fig. \ref{Fig:wisp_snr_mskd}) make colors in this area very unreliable. ... The values shown here are typically a factor of ~3 less than those calculated for the Schmidt data, shown in Figure \ref{Fig:bj_alpha}. ...

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• National Astronomy and Ionosphere Center (Arecibo Observatory)
• Research Areas National Astronomy and Ionosphere Center (Arecibo Observatory)
• The Pleiades

Next: To produce a region Up: Image Display in Xwindows Previous: General usage. ... Menu items are chosen by clicking any mouse button (cf. ... save current cursor as an include region (counts within region will be included in subsequent calculations) . ... When another image is displayed, the earlier one can be compared with it by pressing its respective mouse button with cursor in the main display window. ... Table 1: Detailed list of menu options . ... color . ... enter/leave region sub-menu . ...

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• Region Names and Colors
• ChaMPlane data_archive_.html
• Chandra Images for G007.5-01.7

... The star formation history of NGC 6231 appears to be bi­modal, with a first wave of star formation activity 3--5 Myr ago, followed by a new generation of stars forming # 1 Myr ago. ... Star Formation, Pre­main sequence Stars, Open clusters and associations The star formation history of the rich open cluster NGC 6231 has been hotly debated in the literature ever since the suggestion by Eggen (1976) that a violent process must have triggered star formation in the region. ...

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• ESO - star07
• AdelePlunkettAstro
• ESO - Thesis Topic: Dynamical models of multiple globular cluster populations

... In the nuclear area of the galaxy within the ring, the nucleus appears elongated, and a fainter 3rd star-like component is discernable. ... The 'yellowy' halo about the off-centre nucleus of the ring galaxy is likely composed of redder stars, while the color-neutral nucleus doesn't appear distinctly different in color than either of the ring 'impactor' candidates at bottom center and top right of the picture. ... If so then why are the bright regions within the ring apparently color neutral? ...

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• Combined IRAC2 vs HST Color-Magnitude Diagrams of Bulge Globular Clusters.
• Dusty HII Regions and Planetary Nebulae
• ST ScI Preprint #1362

... Young stellar clusters in the star forming region NGC 6357 . ... A detailed study of the young stellar population in NGC6357, and in Pismis 24 in particular, is presented in the article " Young open clusters in the galactic star forming region NGC 6357 " (Astronomy & Astrophysics, in press) led by Fabrizio Massi (INAF-Observatory of Arcetri) and including Andrea Giannetti (INAF-IRA Bologna), Maria Teresa Beltran (INAF-Observatory of Arcetri) and collaborators in Bologna, Teramo and Chile. ...

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• G35.20-1.74 (Abstract)
• Serpens FCRAO (Abstract)
• APOD: June 25, 1996 - A Star Forming Region in the LMC

. Left panel: The distribution of galaxies 12.7 billion years ago. White circles represent the galaxies, and their size represents the luminosity of the galaxies. The color contour represents the density; the redder the color, the higher the density. The reddest region appears in the lower part of the figure. Right panel: An enlargement from the map that shows the area around the cluster. Credit: NAOJ

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• Why do some stars appear to flash a variety of different colors when you look
• Airborne observatory views star-forming region W40 | Astronomy.com
• Mysterious phenomena in a gigantic galaxy-cluster collision | Astronomy.com

... Current APO Weather . ... Search Site . ... Information for New Users . ... Technical Staff pages . Night Logs and Mailing Lists (maintained by APO) . ... Technical Documents and Database Search . ... Observer's Documentation and Procedures . ... Problem Reporting and APO Technical Documents Database Search . ... APO Drawing/Document Management Procedures . ... APO Technical Documents Database Search . Home Astrophysical Research Consortium . ... Mail Lists (maintained by APO) . ...

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• Astrophysical Research Consortium - Apache Point Observatory
• Night Side of Venus

... About ATNF overview . ... Australia Telescope Steering Committee . ... LMC H II Region Luminosities versus . Observed Ionizing Stars . ... These values are compared to the observed H II region luminosities, yielding an estimate for the mean fraction of H-ionizing photons that escape the local nebulae in this sample. We formally estimate that, overall, 0-51% of the ionizing radiation escapes the local H II regions and is available to ionize the warm, ionized medium in the LMC. ...

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• The giant HII region NGC 3603
• A Blind HI Survey in the Great Attractor Region.
• ATNF Colloquium

... Bad Astronomy . ... Bitesize Astronomy . ... Last week's Snack talked about how black holes can affect the environment around them in such a way as to be very bright . ... It's a common misconception that black holes always have matter swirling into them. ... As this matter gets closer and closer to the black hole it piles up and a large, fairly flat disk forms. This is called the accretion disk , because matter from this disk accretes (that is, falls in) on the black hole. ... 2008 Phil Plait. ...

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... Structure of Data . ... Catalog . ... The SAI OCL Catalog site provides several VO-enabled modes of operation: . VO-enabled catalog data analysis from a browser . ... Endpoint URL is http://ocl.sai.msu.ru/catalog/conesearch/ . ... VO-enabled catalog analysis from a browser . Presently, this recipe works with Firefox (Windows, MacOS, Linux), Internet Explorer (Windows) and Opera (Windows) browsers with Java plugin 1.6 installed. ... Main TOPCAT window with SAI OCL catalog loaded will appear. ...

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• SAI OCL Catalog Publications

... The Milky Way in the region of the Southern CтАж . ... Title: The Milky Way in the region of the Southern Cross (Crux) and Centaurus rising in the south-east behind the 24-inch dome . ... The Milky Way in the region of the Southern Cross (Crux) and Centaurus rising in the south-east behind the 24-inch dome NOTE: All images are copyright and must not be reproduced or mirrored in any form without written permission. ...

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• IAU Commission #34 (Interstellar Matter)
• GSAOI Orion Nebula Cluster Science Page
• VV29 = Arp 188 = The Chainsaw Galaxy

... Basic Research results General information Main characteristics of the Radio telescope Observing programs General view of the antenna array Main research areas Principle of generation of radio images Radio telescope's beam Receiving systems Main characteristics of the base receiving-recording complex Calibrations Data archive and databases Publication of data Possibilities of observing the structure and dynamics of microwave activity SSRT - Research results . ...

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. Pulkovo Observatory of Russian Academy of Sciences is situated . near Saint-Petersburg. It was founded in 1839. 196140, Saint-Petersburg, Pulkovskoye chaussee 65/1 . English version . Russian version . This page has been accessed times since May 1, 1999.

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Astronotes Armagh Planetarium's Stellar Blog! ... Stars . ... Telescopes and Observatories . ... The majestic star-forming region in the Lagoon Nebula. The pale ring to the right is an internal reflection in the telescope.€а (Image credit: ESO/ VPHAS+/ V. Kalari and J. Vink (Armagh Observatory) . ... The 18 component images were further processed twice. ... Venu and his colleagues use images like this to identify individual young forming stars in the Lagoon Nebula and determine their ages. ...

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• Six glorious spiral galaxies seen by the European Southern Observatory. |
• NGC4666: Secrets of a Starburst Galaxy | Astronotes
• Hubble shows us a spectacular star cluster | Astronotes

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19. SAO RAS home page

20. Astronomy HyperText Book: Stellar Clusters