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    1. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/EggNebula.txt
    ... our understanding of how red giant stars transform themselves into planetary nebulae ... 000 year-old history of mass-ejection in a red giant star in such exquisite detail ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/EggNebula.txt -- 5.9 Кб -- 30.01.2001
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    2. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ViaLattea/9830.txt
    ... Red stars come in two flavors: small stars and "red giants". ... Red giant" stars are at the end of their lives because they have exhausted their ... Although many "red giant" stars may have been ordinary stars like our Sun, as they ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ViaLattea/9830.txt -- 2.5 Кб -- 04.03.2001
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    3. APOD: July 9, 1999 - NGC 7789: Galactic Star Cluster
    ... from main sequence stars like the sun into the gaggle of red giant stars apparent (with a reddish-yellow cast) in this lovely ...
    [ 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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    4. APOD: September 17, 1999 - M3: Half A Million Stars
    ... M3's many cool "red" giant stars take on a yellowish cast in this lovely composite image while hotter giants and pulsating variable stars look light blue. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ViaLattea/m3_mochejska_big.html -- 4.2 Кб -- 02.03.2001
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    5. APOD: October 2, 1999 - Phi Persei: Double Star
    ... was actually the most massive star in the system and because of its greater mass evolved into a giant star more quickly ... million years, the roles may reverse as the now massive star swells into its own giant phase "returning" mass to its companion ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/phiper_bpounds_big.html -- 4.8 Кб -- 02.02.2001
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    6. K-band Arcetri Obscured Supernova Search - SNe Intro
    ... inside a binary system consisting of a white dwarf star and an evolving giant star, which results in a termonuclear explosion ... The mass transferred from the giant star increases the mass of the white dwarf to a value higher than the critical limit ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/SNe/intro.html -- 10.7 Кб -- 02.10.2008
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    7. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Hourglass.txt
    ... stars get old, they become cooler and redder, increasing their sizes and energy ... systems like ours) in the universe is manufactured and dispersed by red giant stars ... When the red giant star has ejected all of its outer layers, the ultraviolet ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Hourglass.txt -- 4.9 Кб -- 30.01.2001
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    8. Cannibal Stars Cause Giant Explosions in Fornax Cluster Galaxy (ESO Press
    ESO PR Photo 18b/00 . ... Caption : Images of two of the novae in NGC 1316 that were discovered during the observational programme described in this Press Release. ... In particular, no less than four novae were detected in a single giant galaxy within...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/aggiunta/ESO_orione.htm -- 8.6 Кб -- 29.03.2002
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    9. STScI PRC99-30: Hubble Spies Giant Star Cluster Near Galactic Center
    STScI-PRC99-30 . ... 2 Micron All Sky Survey (2MASS) mosaic of the center of the Milky Way . Credit: University of Massachusetts and Infrared Processing and Analysis Center . ... STScI | ... AURA) , for NASA , under contract with the Goddard Space...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ViaLattea/sgrhorizon.html -- 8.9 Кб -- 04.03.2001
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    10. Arcetri Star-Formation Group Publications
    ... On the nature of Lithium-rich giant stars: constraints from Beryllium abundances . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/starform/publ2005.htm -- 11.6 Кб -- 29.11.2005
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