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    61. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/Edge.txt
    ... NGC 4013 is a spiral galaxy, similar to our own Milky Way, lying some 55 million light-years from Earth in the direction of the constellation Ursa Major. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/Edge.txt -- 5.6 Кб -- 04.03.2001
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    62. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/tagliate/NGC1365a-b.txt
    ... images in visible and infrared light reveals how the barred spiral galaxy NGC 1365 is feeding material into its central region ... A barred spiral is characterized by a lane of stars, gas, and dust slashing across a galaxy's central region. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/tagliate/NGC1365a-b.txt -- 3.7 Кб -- 04.03.2001
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    63. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/0104a.html
    ... UNIVERSE . The central region of the "star-burst" spiral galaxy, NGC . 3310, shows young and old stars evenly distributed. If this were the . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/0104a.html -- 2.6 Кб -- 10.04.2001
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    64. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/QSO100000.txt
    ... Steidel also was somewhat surprised to discover that the galaxy is an elliptical, rather than a spiral. ... The "disturbed-looking" double spiral galaxy above the quasar also is in the foreground. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/QSO100000.txt -- 3.5 Кб -- 04.03.2001
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    65. http://www.arcetri.astro.it/~filippo/snrate08/Contributions_files/ruiter.pdf
    ... with Mtot > 1.4 M (Livio & Riess 2003) Calibration: SN Rates two model galaxies · · · · · · Two simple galaxy models: spiral & elliptical Spiral Galaxy: Z=0.02, constant star formation history for 10 Gyr Elliptical Galaxy: Z=0.002, starburst at t=0 Kroupa ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~filippo/snrate08/Contributions_files/ruiter.pdf -- 1586.3 Кб -- 03.06.2008
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    66. One Hundred Thousand Galaxies at a Glance (ESO PR Photos 46a-j/99)
    ... PR Photo 46i/99 is of a typical spiral galaxy and PR Photo 46j/99 shows another with a strange structure, also in this field. ... In addition, there are many spiral galaxies ; two are shown in PR Photo 46i/99 and PR Photo 46j/99 . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/phot-46d-99-normal.html -- 31.1 Кб -- 21.01.2002
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    67. http://www.arcetri.astro.it/science/k20/papers/0411768.ps
    ... universe approximately 65% of all galaxies are spirals, 32% are ellipticals and 4 ... The shaded regions show the con dence interval for irregulars and spirals galaxies. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/science/k20/papers/0411768.ps -- 2320.7 Кб -- 30.11.2004
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    68. The Solar System
    ... stars visible on a clear night, orbits the center of our home galaxy, a spiral disk of 200 billion stars we call the Milky Way ... It is a spiral galaxy like the Milky Way but is 4 times as massive and is 2 million light years away. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/irlab/Astro/solar/eng/solarsys.htm -- 19.4 Кб -- 15.03.1998
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    69. Fine Shades of a Sombrero (PR Photos 07a-c/00)
    ... This is certainly true for this new image of the famous early-type spiral galaxy Messier 104 , widely known as the "Sombrero" (the Mexican hat) because of its particular shape. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/phot-07b-00-fullres.html -- 4.5 Кб -- 21.01.2002
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    70. http://www.arcetri.astro.it/~sperello/aa535_A13.pdf
    ... to-gas mass ratio and metallicity gradients in four Virgo spiral galaxies L. Magrini1 ,S.Bianchi1 , E. Corbelli1 , L. Cortese3 ... Key words. galaxies: spiral ­ galaxies: abundances ­ submillimeter: galaxies ­ galaxies: ISM ­ dust, extinction 1. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/aa535_A13.pdf -- 497.0 Кб -- 12.01.2012
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