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| | Cosmic Voyage-The Online Resource for Amateur Astronomers |
 | | M102 is relatively bright at 9.8 magnitude and displays an unmistakable lenticular shape across a 4'x1' area. | | | The brightest nearby star to M102 is 5.2 magnitude SAO 29407, 1.2 degrees due south. | | | The closest 6th magnitude star to NGC 5866 is 6.9 magnitude HD 133666, about 31' to the northwest, close enough that inclusion a description for this object would make sense. |
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http://members.aol.com/billferris/m102.html
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| | Galaxy Images |
| | NGC 891 Galaxy in Andromeda (47KB) CCD image taken with an ST-8E CCD using a Takahashi FCT-150 refractor at prime focus on August 26, 2001. | | | M64 The Black-Eye Galaxy (11KB) CCD image taken with an ST-8E CCD using a Takahashi FCT-150 refractor at prime focus on December 13, 2004. | | | M84 and M86 Galaxies in the heart of the Virgo galaxy cluster (20KB) (January 13, 15 and 16, 2005) An RGB color CCD image taken with an ST-8E CCD using a Takahashi FCT-150 refractor with a reducer at f 5.9. |
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http://members.cox.net/sidleach/list_galaxy.htm
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| | gasflow2.html |
| | A series of simulated collisions between a gas-rich disk galaxy and a gas-free elliptical were generated by Gerber (1993), who derived the simulation code from the combined n-body/smoothed particle hydrodynamics code of Balsara (1990). | | | The mass ratio between the elliptical and the disk galaxy (which includes halo, stellar disk, and gas disk components) was varied between 1:1 and 1:10. | | | The unit of time is such that for a Milky Way-size disk galaxy, one computational time unit is approximately 2 Myr. |
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http://www.physics.uiuc.edu/Research/CTA/collide/gas/gasflow2.html
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| | A Visit to Ares Galaxy - addict3d.org |
| | The Ares homepage recommends Ares Lite for Windows 98 users, so this analysis is of Ares, which Windows XP users are instructed to use. | | | Ares Lite has fewer features than Ares, but has a smaller footprint as a result. | | | This leaves the option of Ares, or Ares Lite. |
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http://addict3d.org/index.php?page=viewarticle&type=news&ID=2535
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| | False Ares Prophecy - FileSharing Talk |
| | On the contrary, the entire return query page is listed with various Ares programs; Ares Galaxy FasterDownload 2.2, Ares Fileshare 1.1 (currently unavailable) and the dubious Ares Glaxy Classic 2.0. | | | Ares Galaxy Classic 2.0, developed by "P2P Innovative" is the exact same program as the original Ares Galaxy created by Alberto Treves, save for a few tool bar icon graphics. | | | One in particular is Ares and Ares Lite. |
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http://filesharingtalk.com/vb3/t97715.html
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| | 5.02: electrosphere |
| | But his favorite dumpster is located behind the U of I computer lab. | | | Hanging around the university's computer lab after graduation, he dreamed of a universal digital library and posted an e-text manifesto that grew into Project Gutenberg. | | | "Gutenberg has finally allowed blind people to begin building up libraries of their own," says Churcher, who likes the project so much she has helped scan in 12 books, including The Pickwick Papers, for Gutenberg's files. |
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http://www.wired.com/wired/archive/5.02/esgutenberg_pr.html
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| | Galaxy |
| | Galaxy classification Galaxy classification is put galaxies into different categories based on their characteristic shap... | | | The Hitchhiker's Guide to the Galaxy (computer game) The Hitchhiker's Guide to the Galaxy is a IBM PC. | | | The Hitchhiker S Guide To The Galaxy Computer Game |
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http://www.brainyencyclopedia.com/topics/galaxy.html
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| | Galaxy Images |
| | NGC 891 Galaxy in Andromeda (47KB) CCD image taken with an ST-8E CCD using a Takahashi FCT-150 refractor at prime focus on August 26, 2001. | | | NGC 3628 Galaxy in Leo (13KB) CCD image taken with an ST-8E CCD using a Takahashi FCT-150 refractor at prime focus in March 2004. | | | M84 and M86 Galaxies in the heart of the Virgo galaxy cluster (20KB) (January 13, 15 and 16, 2005) An RGB color CCD image taken with an ST-8E CCD using a Takahashi FCT-150 refractor with a reducer at f5.9. |
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http://members.cox.net/~sidleach/list_galaxy.htm
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| | Shropshire Astronomical Society - Deep Sky Images page |
| | On the image on the left the galaxy appears to be about 9' long only just fitting in the field of the 8" scope and TC255 based CCD camera I used. | | | This relatively bright face on barred spiral galaxy M95 is to be found in Leo not far from M96. | | | This image was taken by Kev Wildgoose using a 12" Newtonian and MX916 CCD camera. |
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http://www.astro.cf.ac.uk/sas/galaxy.htm
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| | Martin White: Probes of Large Scale Structure |
| | Galaxy surveys with well defined selection criteria enable us to extract information about the clustering pattern. | | | They are found to lie in clusters, filaments, bubbles and sheet like structures.) In the early 1980s there were less than 5,000 galaxy redshifts known. | | | The VIRMOS-VLT Deep Survey (VVDS) project on the VLT. |
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http://astron.berkeley.edu/~mwhite/probes-lss.html
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| | Essays Page |
| | If indeed any of these MACHO candidates does turn out to be the main component of the dark matter, scientists will have the difficult task of explaining why such large numbers exist in galaxy halos. | | | The earliest suggestion that a large amount of the material in the universe might be undetectable, or dark, matter came with the work of Fritz Zwicky (1898–1974) in the 1950s. | | | Such objects do exist; neutrinos (elementary particles with no charge or mass) are a good example of objects that are nearly impossible to detect, yet exist in large numbers. |
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http://www.fofweb.com/Subscription/Science/Helicon.asp?SID=2&iPin=ffests0235
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| | Galaxies |
| | According to computer simulations, the variety of galaxy forms results from different initial parameters of the proto-galaxies such as the amount of (initial) angular momentum, as well as their later evolution in their environments, such as interaction with other neighboring galaxies. | | | Occasionally, at irregular intervals given by chance, in any type of galaxies, a supernova occurs: This is a star suddenly brightning to a high luminosity which may well outshine the whole galaxy; the maximal absolute magnitude of a supernova may well reach -19 to -20 magnitudes. | | | However, for some ellipticals, small disk components have been discovered, so that they may be representatives of one end of a common scheme of galaxy forms which includes the disk galaxies. |
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http://www.seds.org/messier/galaxy.html
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| | [7.0] Beyond The Milky Way |
| | Galaxies with unusual and puzzling features are sometimes given a secondary classification as "peculiar". | | | However, they were extremely bright, roughly a thousand times brighter than galaxies observed at comparable distances, and more interestingly, their brightness varied rapidly, sometimes changing by an order of magnitude in days. | | | Ellipticals range in size from very small dwarf ellipticals to supergiants, with the supergiants an order of magnitude larger than the Milky Way. |
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http://www.vectorsite.net/tastga7.html
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| | Andromeda |
| | There are a number of fine binaries and several variables, and some very nice deep sky objects, including perhaps the most famous spiral galaxy of all. | | | One of Andromeda's greatest attractions is the spiral galaxy known as M 31. | | | This galaxy is located almost half a degree to the south of M31 and is best seen in large telescopes. |
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http://www.dibonsmith.com/and_con.htm
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| | Dark Matter and Galaxy Clumping |
| | Tyson finds that dark matter follows the overall pattern of visible matter but that its basic unit of 'clumpiness' measures about 300,000 light-years across, distinctly larger than a typical galaxy. | | | The object is so far away, observing it in such detail would tax the capabilities of both Hubble and Keck without the magnification of the gravitational lens, provided by a foreground cluster of galaxies that is much closer to us at 5 billion light-years. | | | The distribution of galaxies in the Hubble Deep Field images may yield clues to the curvature of space. |
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http://www.dhushara.com/book/quantcos/dark/dark.htm
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| | Ares P2P - Join the Future of P2P File Sharing |
| | This is especially useful when you allow other family members to use Ares P2P on your computer. | | | However, the best way to keep your computer protected is to always scan new files with an up-to-date virus scanner. | | | The first step in solving connection problems is to make sure your computer is connected to the Internet. |
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http://www.aresp2p.net
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| | Ares FAQ--READ BEFORE POSTING ANY QUESTIONS - Peer Evolution Forums |
| | The best (and easiest) solution will be to uninstall Ares from your computer, restart your computer, Then DL a new copy from the site Ares Install this new copy to your computer and everything should be solved. | | | Ares downloads from more than one source at a time, this lets you know what parts of the file you currently have, and what parts you don't. | | | If you're not using your own computer, or you are not the administrator for the computer, there could be a privilege setting or some other block to make sure certain things aren't DL'ed to the computer (especially school computers). |
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http://www.peerevolution.com/forums/showthread.php?t=126
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| | Investigating the Evolution of Quasar Host Galaxies with NICMOS |
| | This implies quasar:host ratios and galaxy luminosities which are consistent with the values obtained for low- z objects, although the uncertainties are currently too large to allow the testing of specific models of galaxy evolution. | | | Host galaxy studies are currently one of the most promising avenues of inquiry since they hold out the hope of linking quasars into the latest models of galaxy formation and evolution. | | | Given that the host galaxies of low-redshift quasars have properties consistent with the products of successive galaxy mergers, and given the dramatic cosmological evolution seen in the quasar population (see below) one of the key aims of new quasar research must be to investigate the cosmological evolution of their hosts. |
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http://ecf.hq.eso.org/instruments/nicmos/sardinia/node34.html
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| | SAI Supernova catalog |
| | Galaxy CGCG 064-024 is also close to the supernova position. | | | The recession velocity of supernova's parent galaxy is known with a big uncertainty. | | | The host galaxy "NGC 6240" = "PGC 059186" is disfigured. |
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http://www.sai.msu.su/sn/sncat/remarks.html
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| | The Gutenberg Galaxy - Alison Harwood |
| | The Gutenberg Galaxy exemplifies one of Dennett’s algorithmic processes. | | | The Gutenberg Galaxy is a valuable stimulant to thought about modern communications technology. | | | The Gutenberg Galaxy is enlightening, provocative and stimulating. |
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http://users.bigpond.net.au/marshan/book5.htm
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| | GSAOI Dwarf Galaxies Science Page |
| | For example, among the Galaxy's companions there is a tendency for the systems with stronger intermediate-age components to lie at larger Galactocentric distances. | | | To make progress in understanding the processes that govern dwarf galaxy evolution, we need to study systems beyond the Local Group. | | | The existence of this system demonstrates that proximity to a large galaxy cannot be the only factor governing the evolution of dwarf galaxies. |
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http://msowww.anu.edu.au/gsaoi/science/dwarfs.shtml
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| | GIC - 3314 collision, striations, dopplers, cartwheel |
| | Galaxy theorists attempting computer simulations regards the formation of galaxies and galaxy arms cannot begin to home in on the answer until bi-lateral symmetry is understood enough to be correctly incorporated into their modelling equations. | | | In galaxies, the curled fingers can be long reaching, reaching all the way around to the other side of a galaxy, even longer, whorling all the way around a galaxy, but, nevertheless, a finger (arm) sourced in the galaxy originates in just one of the two unique 'handedness' modes possible for curled fingers. | | | Galaxy Ngc 4603 is an excellent galaxy summary example in having enormous quantities of 'missing mass', a tightly wound spiral form that changes into an irregular basin teeming with chaos when viewed in 3D overlay, well exampled s-shaped forms, and dish halo at the core. |
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http://www.cosmicastronomy.com/3314.htm
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| | Ares Gold - The Fastest P2P File Sharing Program |
| | More recent P2P file sharing programs like Kazaa, LimeWire, Ares Galaxy, Morpheus and Grokster, use a decentralized approach by which supernodes, typically individual computers with a broadband Internet connection, take care of routing the search queries over the network. | | | Ares Gold is a free file sharing program that builds on the latest P2P technology to offer a unique and exciting user experience. | | | Within seconds, Ares Gold brings up thousands of MP3s, movies, images, games, and other media files which can be downloaded fast from multiple sources and managed in an easy to use media library. |
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http://www.aresgold.com
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| | Galaxies News Articles |
| | Astronomers call the galaxy the Sombrero because of its resemblance to a Mexican hat and have a special affection for it - it is often seen adorning the walls of observatories and universities all over the world. | | | The Sombrero galaxy has an unusually large and extended central bulge of stars, as well as dark prominent dust lanes that can be see silhouetted against the stars. | | | The smallest galaxy at the center of the image could be related to the other three or an unrelated background object, she said. |
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http://www.crystalinks.com/galaxynews4.html
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| | Sloan Digital Sky Survey |
| | This galaxy is unusual in that the gas in the galaxy rotates counter to the rotation of the stars. | | | NGC 3626 is a spiral galaxy with a striking dust lane encircling its central bulge. | | | The colors of the different parts of the galaxy show differences in star formation history: the reddish color of the central bulge indicates that it is older than the disk, while the blue spots in the disk, particularly in the arms, show where new star formation is taking place. |
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http://www.sdss.org/iotw/archive.html
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| | The Triangulum Transmission |
| | Although the Triangulums cannot be completely sure, they postulate that the unknown creators of the Leviathan have imploded their entire galaxy down to a fraction of its former size before converting it into a single artificial structure or complex of structures and launching it across intergalactic space. | | | This means that virtually all high toposophic-level devices such as wormholes, weylforges and deep-well industrial zones are direct extensions of The Source itself. | | | Although most of their technology has developed in fairly conventional ways, the Eh'ern are recognized within Triangulum civilization for their unique approach to spacecraft and space habitat design. |
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http://www.orionsarm.com/xenos/Triangulum_Transmission.html
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| | GIC - 3314 collision, striations, dopplers, cartwheel |
| | Galaxy theorists attempting computer simulations regards the formation of galaxies and galaxy arms cannot begin to home in on the answer until bi-lateral symmetry is understood enough to be correctly incorporated into their modelling equations. | | | In galaxies, the curled fingers can be long reaching, reaching all the way around to the other side of a galaxy, even longer, whorling all the way around a galaxy, but, nevertheless, a finger (arm) sourced in the galaxy originates in just one of the two unique 'handedness' modes possible for curled fingers. | | | Galaxy Ngc 4603 is an excellent galaxy summary example in having enormous quantities of 'missing mass', a tightly wound spiral form that changes into an irregular basin teeming with chaos when viewed in 3D overlay, well exampled s-shaped forms, and dish halo at the core. |
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http://www.cosmicastronomy.com/3314.htm
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| | oral.html |
| | Although detection and recognition of such galaxies are not difficult, gathering the wealth of information needed to decipher the physical mechanisms and their role in evolution of diverse galaxy types and environments will require much larger samples and wide wavelength coverage. | | | These observables are compared with the prediction of semi-analytic Cold Dark Matter models for galaxy formation and evolution, of which we have developed a new rendition. | | | The lower proper motion limit of our survey is defined by the initial 5 arcsec matching radius used for the identification of the objects measured on the R- and BJ-plates and by the epoch difference between the plates in a given field. |
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http://www.eso.org/gen-fac/meetings/hdfs2000/oral.html
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