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    81. APOD: October 11, 1999 - Eta Carinae in X Rays
    ... Eta Carinae is the one of the most luminous star systems in our Galaxy , radiating millions of times more power than our Sun ... Pictured above , a horseshoe-shaped outer ring about two light-years across has been discovered surrounding a hot core ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Stelle/etacarina_chandra_big.html -- 4.7 Кб -- 02.02.2001
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    82. Research on AGN
    ... Our group has been studying the co-evolution of AGN, BHs, and their host galaxies for several years now. ... We rely on a multiwavelength approach, from the millimeter and the IR to the X-ray. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/ricerca/galassie-agn-cosmologia/211-ricerca/galassie/838-agn -- 33.9 Кб -- 11.04.2016
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    83. The first ultraviolet average spectrum of z=2.4 quasars
    ... below 1216 У? (the rest-frame wavelength of LyЮБ emission in the quasar spectrum) is due to absorption from the IGM, which attenuates the quasar flux, both in the Lyman series (creating the so-called HI forest), and in the Lyman continuum at rest ЮЛ<912 У ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/previous/204-scientific-news/829-qso-uv-spectrum -- 28.1 Кб -- 10.04.2016
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    84. Hotels Zona Osservatorio
    ... Research . Adaptive Optics . Galaxies, AGN, Cosmology . High energy . Infrared astronomy . Optical turbulence . ... Fri. 9.30-13.30/14.30-17.30 but possible also to ring Mr Carlo Quinterio (owner) at cell ph. 335/6363 033 . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/about-us/how-to-reach-us/179-informazioni/251-hotels-zona-osservatorio?showall=&start=1 -- 30.7 Кб -- 12.04.2016
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    85. APOD: May 24, 1996 - In the Center of 30 Doradus
    ... 30 Doradus and R136 lie in the LMC - a satellite galaxy to our own Milky Way Galaxy . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/30doradus_hst_big.html -- 4.3 Кб -- 04.03.2001
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    86. http://www.arcetri.astro.it/~sperello/ASPCS374_449.pdf
    ... how the star formation history of ETG depends on the galaxy mass and the environment, we are proposing a different approach (di ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/ASPCS374_449.pdf -- 224.1 Кб -- 21.12.2007
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    87. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Hen.txt
    ... The images that Bobrowsky and collaborators acquired show a ring of gas surrounding the central star, with bubbles of gas above and below the ring. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/Hen.txt -- 6.4 Кб -- 30.01.2001
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    88. http://www.arcetri.astro.it/science/k20/papers/0409041.ps
    ... technique for selecting Lyman­Break Galaxies (LBG, Steidel et al. 1996; 2003) from their U n GR s rest­frame UV colors, which ... SFRs from the Rest­Frame UV­Continuum Luminosity Estimating the SFR of a galaxy from its multicolor optical photometry is ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/science/k20/papers/0409041.ps -- 1598.8 Кб -- 30.11.2004
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    89. http://www.arcetri.astro.it/igm50/talks_all/crighton.pdf
    ... It provides a useful constraint for theoretical models of galaxy formation (Lagos+ 2011, Dave+ 2013, Popping+ 2014, Rahmati ... Low resolution spectra (~300 km/s FWHM) covering rest frame 912-1300 A with SNR ~20. 5 z=0.2 z=1.3 Finding DLAs becomes ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/igm50/talks_all/crighton.pdf -- 2216.1 Кб -- 17.06.2015
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    90. http://www.arcetri.astro.it/~sperello/AA574A126.pdf
    ... galaxies, and 39 spirals ranging from early to late types, that we will use ... filled dots), galaxies with 0.5 Def HI < 0.9are Hi-deficient (rings), and those with ... galaxies as given by the Hi deficiency parameter: Hi-normal (filled dots), Hi ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/AA574A126.pdf -- 2270.9 Кб -- 04.03.2015
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