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1. APOD: 2001 February 7 - Distant Open Cluster M103
... 2001 February 7 . Distant Open Cluster M103 . ... Explanation: Bright blue stars highlight the open cluster known as M103 . The gas clouds from which these stars condensed has long dispersed. ... In fact, a formerly blue star has recently evolved off the main sequence and is visible above as the red giant star near the cluster center. In general, yellow stars like our Sun are usually less bright and hence less prominent in open clusters than their massive blue cousins. ... About APOD | ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap010207.html -- 5.2 Кб -- 01.10.2012
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2. M100: A Grand Design
... M100: A Grand Design . ... Credit: NASA Explanation: Majestic on a truly cosmic scale, M100 is appropriately known as a Grand Design spiral galaxy. A large galaxy of over 100 billion or so stars with well defined spiral arms , it is similar to our own Milky Way . One of the brightest members of the Virgo Cluster of galaxies , M100 (alias NGC 4321) is 56 million light-years distant in the spring constellation of Coma Berenices . ... Publications with keywords: M100 - spiral galaxy . ...
[ Сохраненная копия ]  Ссылки http://www.astronet.ru/db/xware/msg/apod/2001-02-03 -- 13.9 Кб -- 02.02.2001
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3. Simulation of a Distant Cluster of Normal Galaxies
... We have simulated the observations of a very distant cluster of galaxies at high redshift. ... The simulations are made for the HST instruments FOC, WFPC II, and the Advanced Camera, and for an 8-m telescope on the ground equipped with adaptive optics. ... A comparison of the fields of view of post-COSTAR HST imaging instruments with the Advanced Camera (AC) and the ground-based adaptive optics camera (AO) is shown in Fig. 1 superimposed on the noise-free cluster simulation. ...
[ Сохраненная копия ]  Ссылки http://www.stsci.edu/stsci/meetings/irw/proceedings/cauleta.dir/section3_2.html -- 11.5 Кб -- 15.04.1994
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4. APOD: July 9, 1999 - NGC 7789: Galactic Star Cluster
... July 9, 1999 . NGC 7789: Galactic Star Cluster . ... Explanation: At 1.6 billion years old, this cluster of stars is beginning to show its age. NGC 7789 is an open or galactic star cluster about 8,000 light-years distant toward the constellation Cassiopeia and lies near the plane of our Milky Way galaxy. ... These have evolved from main sequence stars like the sun into the gaggle of red giant stars apparent (with a reddish-yellow cast) in this lovely composite color image. ... About APOD > . ...
[ Сохраненная копия ]  Ссылки http://www.sai.msu.su/apod/ap990709.html -- 4.8 Кб -- 02.10.2012
[ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ViaLattea/ngc7789_mochejska_big.html -- 4.7 Кб -- 02.03.2001
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5. The Pleiades
... The Pleiades star cluster, also known as the Seven Sisters and Messier 45, is a conspicuous object in the night sky with a prominent place in ancient mythology . ... The stars in the Pleiades are thought to have formed together around 100 million years ago, making them 1/50th the age of our sun, and they lie some 130 parsecs (425 light years ) away. ... Data for these stars are listed in a table below. ... Yes . ... WEBDA Pleiades cluster data . ... M45: The Pleiades Star Cluster (2007 November 18) ...
[ Сохраненная копия ]  Ссылки http://www.naic.edu/~gibson/pleiades/ -- 29.7 Кб -- 07.02.2015
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6. Improvements in Filter Design for Removing Galactic ``Cirrus'' from IRAS Images
... Next: Star Finding and Up: Image Restoration and Previous: Multiresolution and Astronomical . ... Design improvements continue to be made in the filter developed using mathematical morphology principles for the Infrared Astronomical Satellite ( IRAS ) images. The purpose of this filter is to eliminate Galactic cirrus emission from extragalactic fields. ... With an appropriate normalization, the filter curve was applied to each pixel in the image to remove the Galactic cirrus. ...
[ Сохраненная копия ]  Ссылки http://www.adass.org/adass/proceedings/adass94/basartj.html -- 11.6 Кб -- 03.11.2000
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8. Armagh Observatory
... a spiral galaxy some million light years away, made by combining images . ... 1st February using the Armagh Robotic Telescope at the Armagh Observatory. ... Image credit: Simon Jeffery. Astronomers Simon Jeffery and Jack Wright have obtained their first images of deep-space objects using a new тАЬroboticтАЭ telescope at Armagh Observatory. ... Simon Jeffery, project scientist for the new telescope, said: "After two years of hard work, it is very satisfying to see the first images looking so good. ...
[ Сохраненная копия ]  Ссылки http://star.arm.ac.uk/press/2011/csj_telescope01_revised.html -- 8.7 Кб -- 04.02.2011
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9. Wonders of the February Night Sky | Astronotes
Astronotes Armagh Planetarium's Stellar Blog! ... Moon . Planets . ... Monthly Sky Notes . ... February . ... The ringed planet will be quite bright, but unlike Jupiter it will not be the brightest point of light in the sky, this accolade will return to Sirius which is the brightest star in our night sky in the constellation of Canis Major. ... Seven days later on February 18, the Moon will be in its full Moon phase. ... Tweets that mention Wonders of the February Night Sky | ... Astronotes . ...
[ Сохраненная копия ]  Ссылки http://www.armaghplanet.com/blog/wonders-of-the-february-night-sky.html -- 46.5 Кб -- 09.04.2016
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10. ASP: Star Science in the Autumn Sky
In autumn 1994, two groups of astronomers announced that they had discovered Cepheid variable stars in a distant cluster of galaxies. ... As the term suggests, variable stars change in brightness over time. ... Variable stars are an ideal way to get high-school students doing real science, with real data, from the real sky. ... a sky chart to find the stars . ... Students can use the nearby stars to estimate the magnitude of Delta. ... Locate the star Delta in Cepheus and estimate its brightness . ...
[ Сохраненная копия ]  Ссылки http://www.astrosociety.org/edu/publications/tnl/32/starscience3.html -- 13.5 Кб -- 02.10.2012
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11. Southern SHARC survey
... This paper ( Burke et al. 2003 ) describes the creation of one such catalogue - the Southern Serendipitous High-redshift Archival ROSAT Cluster (SHARC) survey - which covers an area of 17.7 deg 2 and consists of 32 clusters with redshifts between 0.05 and 0.7 and X-ray luminosities between 7 x 10 42 and 4 x 10 44 erg/s: the high-redshift subsample contains 16 clusters with = 0.3 and X-ray luminosities greater than 2 x 10 43 erg/s (luminosities are quoted for the 0.5 - 2.0 keV energy band). ... 1997 ...
[ Сохраненная копия ]  Ссылки http://hea-www.harvard.edu/~dburke/southern_sharc/ -- 7.8 Кб -- 01.10.2012
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12. http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBC8EF0A5-0360-4884-8A71-93C4AD539C7C%7D
XMM-Newton observation of the core of the massive cluster Cyg OB2 located in the constellation Cygnus, 4,700 light-years from Earth. The cluster contains massive O-type stars that shine brightly in X-rays. Cyg OB2 #9 is seen as the bright star just below the central star, and in 2008 was determined to be a binary system. ... Hundreds of lower mass stars also fill the field of view, which spans nearly 22 x 16 arcminutes. ...
[ Сохраненная копия ]  Ссылки http://www.astronomy.com/sitefiles/resources/image.aspx?item=%7BBC8EF0A5-0360-4884-8A71-93C4AD539C7C%7D -- 4.2 Кб -- 10.04.2016
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13. This MonthтАЩs Sky тАУ February 2016 ? Amateur Astronomers Association of New
... Home Observing This Month?s Sky This MonthтАЩs Sky тАУ February 2016 . ... This MonthтАЩs Sky тАУ April 2016 . This MonthтАЩs Sky тАУ March 2016 . This MonthтАЩs Sky тАУ February 2016 . ... Beyond New York City . ... Observing Resources for Amateur Astronomers - Part 1: Beginning Observers . ... A History of the First Forty Years of the Amateur Astronomers Association . ... Amateur Astronomers Medal . ... 2016 Amateur Astronomers Association of New York Designed by Press Customizr Powered by . ...
[ Сохраненная копия ]  Ссылки http://www.aaa.org/observing/this-months-sky/this-months-sky-february-2016/ -- 103.5 Кб -- 10.04.2016
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14. http://www.mso.anu.edu.au/~bessell/thumbnails/images.txt
GALAXIES cenA .tiff 40 Bright Radio Galaxy M31.tiff Nikon Andromeda Galaxy (note HII regions in spiral arms) ngc6744.tiff 40 NGC 6744 a face-on spiral clouds_20d.tiff H'blad The Magellanic Clouds our nearest neighbours Lmc_7.tiff Nikon The Large Magellanic Clouds Lmc_zoom.tiff Nikon Detail of previous image smc_7.tiff Nikon The Small Magellanic Clouds smc-zoom.tiff Nikon Detail of previous image 30dor_40_BVR.tiff 40 The 30 Dor ... B [OIII] Halpha trifid.tiff 40" The Trifid Nebula. ...
[ Сохраненная копия ]  Ссылки http://www.mso.anu.edu.au/~bessell/thumbnails/images.txt -- 8.7 Кб -- 27.01.2004
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15. HIPASS Science meeting
15m) Baerbel Koribalski (ATNF) "The HIPASS Bright Galaxy Survey" . ... 15m) Stuart Ryder (AAO) "HIPASS J0731-69: A New Tidal Feature in the NGC 2442 Group" . ... 15m) Meryl Waugh (U.Melbourne) "The Fornax Region: Searching for Clusters in HIPASS" . ... 15m) Martin Zwaan (U.Melbourne) "Constaints on the Space Density of Intragroup HI Clouds" . ... 15m) Lister Staveley-Smith (ATNF) "Mapping the Magellanic Stream" . ... 15m) Joss Bland-Hawthorn (AAO) "HIPASS HI clouds and the metagalactic UV field" . ...
[ Сохраненная копия ]  Ссылки http://www.atnf.csiro.au/research/multibeam/meet/20010205.html -- 3.1 Кб -- 02.10.2012
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16. Galaxy Gallery Page II
... They cover a period of 4 days in which the Supernova continues to rise in brightness (what astronomers call magntiude). ... First Image Taken on March 11 at 8:22 UT. Second Image Taken on March 12 at 8:52 UT. ... The supernova is the same brightness as in the previous image taken 2 hours ago . ... This image, taken 24 hours after the previous image, shows the supernova to be another 0.21mag (or about 25%) brighter. ... Hopefully the images do show that the brightness of the Supernova is changing. ...
[ Сохраненная копия ]  Ссылки http://zebu.uoregon.edu/sn.html -- 6.3 Кб -- 07.10.1996
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17. NICMOS/HST H-band (F160W) Images of the 30 Dor Starburst Cluster
Next: The Formation and Evolution Up: NICMOS Science Previous: NICMOS Observes the Galactic . ... We have taken diffraction-limited ( 0.15") near-infrared F160W (henceforth H-band, for convenience) images with NICMOS on HST of the center of the R136 cluster (age 3.5 Myr) in the core of the 30 Dor giant HII region in the Large Magellanic Cloud. ... 1996, ApJ 466, 274) can sample only M >2M , while previous V and I band HST images with WFPC2 (Hunter et al. ...
[ Сохраненная копия ]  Ссылки http://www.stecf.org/conferences/sardinia/node26.html -- 13.9 Кб -- 12.06.2006
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18. http://www.mrao.cam.ac.uk/~tm419/downloads/Graduate_student_poster.pdf
The FR Divide in Radio Galaxies through Environmental Interactions T. Maciel (Astrophysics Group) tm419@cam.ac.uk , P. Alexander (Astrophysics Group) Radio -Loud Galaxies · Galaxies which are dominated by their radio emission (10MHz -100GHz) and show extended morphology: - Jets Active Galactic Nuclei -Lobes powered by (AGN) -Hotspots -Central black hole -Accretion disc -Strong B fields -Dusty torus Chandra X-Ray image of Perseus cluster with VLA ... Right: FRII galaxy 3C175 at 5GHz. ...
[ Текст ]  Ссылки http://www.mrao.cam.ac.uk/~tm419/downloads/Graduate_student_poster.pdf -- 2276.9 Кб -- 26.04.2013
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19. Image: Nursing house designed by Brunelleschi. On piazza SS. Annunziata.
. Album : asv-album :: Travels to distant places and countries :: 1999/09 Florence, Rome (Italy) :: 15/09 Piazza SS. Annunziata. Fiesole-Settignano walking tour . Up . << Prev . Nursing house designed by Brunelleschi. On piazza SS. Annunziata. Next >> . Album created by album generator a tool written by Dave on Tue Jun 23 14:47:05 2015 .
[ Сохраненная копия ]  Ссылки http://crydee.sai.msu.ru/album/trips/1999.09.Italy/15.Fiesole-Settignano/tn/c29l.jpg.index.html -- 6.2 Кб -- 23.06.2015
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20. A0690 radio identifications
... RS 1 0.05 Id C # fst 08 39 15.754 +28 51 25.62 11.51 9.9 0.0 159.0 fst 08 39 15.810 +28 51 06.90 13.92 18.7 0.0 174.2 fst 08 39 15.882 +28 50 48.07 27.25 12.6 1.6 3.8 fst 08 39 15.849 +28 50 39.07 124.72 1.1 0.4 178.4 fst 08 39 16.285 +28 52 16.44 W 10.54 13.4 6.5 27.5 fst 08 39 17.780 +28 51 42.03 W 2.12 13.6 -4.1 8.1 fst 08 39 15.665 +28 50 12.85 W 2.02 8.3 -2.8 19.5 fst 08 39 13.364 +28 49 19.12 46.61 25.1 7.6 81.9 ...
[ Сохраненная копия ]  Ссылки http://www.sao.ru/cats/~CLUSTERS/CLUSTERS/RO_images/A0690/A0690id.html -- 10.1 Кб -- 03.03.2001
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