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    1. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ViaLattea/Milk_Radio.txt
    ... our galaxy as seen in visible light shows enigmatic "high-velocity clouds" of gas high above the plane of the Milky Way which ... High-velocity clouds are from the survey done at Dwingeloo Observatory (Hulsbosch & Wakker, 1988).. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ViaLattea/Milk_Radio.txt -- 2.7 Кб -- 04.03.2001
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    2. SECCO1: an "almost-dark" dwarf galaxy
    ... for the stellar counterparts of Ultra Compact High Velocity Clouds (UCHVC) represent a promising approach that already resulted ... HII regions within a compact high velocity cloud. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/previous/204-scientific-news/814-secco1 -- 27.9 Кб -- 10.04.2016
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    3. SECCO1: an "almost-dark" dwarf galaxy
    ... for the stellar counterparts of Ultra Compact High Velocity Clouds (UCHVC) represent a promising approach that already resulted ... HII regions within a compact high velocity cloud. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/precedenti/204-scientific-news/814-secco1 -- 37.7 Кб -- 10.04.2016
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    4. S235 (Abstract)
    ... of S235 A and S235 B. Strong variability of the maser emission and large velocity differences of the maser features with respect to the molecular cloud velocity imply the presence of highly collimated, energetic and short duration jet activity in this YSO ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/s235/abstract.html -- 4.2 Кб -- 11.09.2007
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    5. http://www.arcetri.astro.it/~sperello/AA477_789.pdf
    ... Other mechanisms, such as in-fall of high velocity gas clouds, gas outflows or bars may also contribute to the observed evolution in the kinematics. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/AA477_789.pdf -- 1868.0 Кб -- 23.01.2008
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    6. http://www.arcetri.astro.it/~sperello/arXiv1311.1774.pdf
    ... The upper bound corresponds to the highest velocity in our Herschel detection list of 207 galaxies and the lower bound is set to avoid confusion with Galactic hydrogen and local high velocity clouds. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/arXiv1311.1774.pdf -- 1257.8 Кб -- 08.11.2013
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    7. http://www.arcetri.astro.it/~sperello/MNRAS438_1922.pdf
    ... area that have a velocity of 400 <v Helio < 2659 km s-1 .The upper bound corresponds to the highest velocity in our Herschel detection list of 207 galaxies and the lower bound is set to avoid confusion with Galactic hydrogen and local high-velocity clouds ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~sperello/MNRAS438_1922.pdf -- 1936.2 Кб -- 04.03.2014
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    8. http://www.arcetri.astro.it/~lt/preprints/s235/s235.ps.gz
    ... with respect to the molec­ ular cloud velocity imply the presence of highly collimated, energetic and short duration jet ... The interaction of these high velocity jets with the surrounding molecular cloud may give rise to the masers. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/s235/s235.ps.gz -- 554.0 Кб -- 11.09.2007
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    9. Serpens FCRAO (Abstract)
    ... the denser gas in the cloud cores, previously studied at high angular resolution ... velocity show an increasing, smooth gradient in velocity from East to West, which we ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/ser_fcrao/abstract.html -- 3.2 Кб -- 11.09.2007
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    10. http://www.arcetri.astro.it/igm50/posters_all/armillotta.pdf
    ... The cloud radius is the typical size of the Intermediate Velocity Cloud. 2/3 vir No condensation or evaporation The higher the galaxy virial mass, the higher the coronal temperature the lower the coronal gas condensation. ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/igm50/posters_all/armillotta.pdf -- 1235.5 Кб -- 16.07.2015
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