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    61. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/Minuetto.txt
    ... complex details in the dust lanes of the group's largest galaxy member (HCG 87a), which is actually disk-shaped, but tilted so ... dark bands across the large edge-on disk galaxy are due to interstellar dust silhouetted against the galaxy's background ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/Minuetto.txt -- 4.7 Кб -- 04.03.2001
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    62. http://www.arcetri.astro.it/~lt/preprints/proplyds/proplyds.ps.gz
    ... disks surrounding young stellar objects (YSOs) comes from the infrared excesses, IR ... the dark edge­on disk seen in silhouette has relatively low dust opacity and glows ...
    [ Текст ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/proplyds/proplyds.ps.gz -- 230.3 Кб -- 11.09.2007
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    63. BD_disks (Abstract)
    ... These sources are known from a previous study to be associated with dense gas and dust, and not associated with HII regions. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~lt/preprints/mol_ovro/abstract.html -- 3.4 Кб -- 11.09.2007
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    64. Arcetri Star-Formation Group Publications
    ... 2006, A , in press . Large dust grains in the inner region of circumstellar disks . A. Isella, L. Testi, A. Natta . 2006, A , in press . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/starform/publ2006.htm -- 10.3 Кб -- 14.12.2006
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    65. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/RingGalax.txt
    ... During the collision the gas from the smaller galaxy would have been stripped off and captured by the larger galaxy, forming a new ring of dust, gas, and stars, which orbit around the inner galaxy almost at right angles to the old disk. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/RingGalax.txt -- 6.7 Кб -- 04.03.2001
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    66. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/TwoJets.txt
    ... The jet is seen in visible light, and its dusty disk and stars are seen in infrared light. ... These stars are located near a huge torus, or donut, of gas and dust from which they formed. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/ISM/TwoJets.txt -- 2.9 Кб -- 30.01.2001
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    67. A picture of a Sun-like protostar: the jet, the cavity and the forming disk
    ... The dust continuum imaged by ALMA is я??attened perpendicular to the jet and suggestive of a disk of (maximum) radius т?? 0.3 AU. ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/en/previous/204-scientific-news/768-alma-codella -- 31.2 Кб -- 10.04.2016
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    68. research field
    ... ISM diagnostics for star-formation processes, and structural properties of AGN host galaxies and normal spiral bulges and disks ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/science/gal-agn/res_hunt.html -- 2.8 Кб -- 10.01.2012
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    69. http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/phot-07b-00-fullres.html2
    ... composed primarily of mature stars, and its nearly <i>edge-on disk</i> composed of stars, gas, and intricately structured dust ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/phot-07b-00-fullres.html2 -- 12.7 Кб -- 21.01.2002
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    70. APOD: April 12, 1999 - Nearby Spiral Galaxy NGC 4945
    ... The thin disk galaxy is oriented nearly edge-on, however, and shrouded in dark dust . ...
    [ Сохраненная копия ]  Ссылки http://www.arcetri.astro.it/~palla/ANDREAIMMAGINI/Galassie/ngc4945_mpg_big.html -- 4.9 Кб -- 04.03.2001
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