... Solution requires spectroscopic measurement to identify dust grain features in the protostellar disks, from 8-30µm. Requires high spectral and spatial resolution spectrometers on Antarctic and 8m-class IR telescopes. ...
... We also find a correlation between 21 cm line strength and the optical-near-infrared color, which suggests that the reddening is caused by dust located in the large-scale, H I absorbing disk which intervenes the sight line to the AGN. | ...
... Emonts, B.; Woudt, P. A. "Active disk building in a local HI-Massive LIRG: the synergy between gas, dust, and star formation ... Published (O) 192 *Ricci, L.; Testi, L.; Natta, A.; Brooks, K. J. "Dust grain growth in p-Ophiuchi protoplanetary disks". ...
[
Текст
]
Ссылки http://www.atnf.csiro.au/research/publications/ATNF_Publications_2010.pdf -- 102.0 Кб -- 08.03.2011 Похожие документы
... Helene Roussel (MPIA) SINGS team: Warm molecular hydrogen in nearby galaxies: excitation mechanisms and link with dust heating ... Anil Seth , Roelof de Jong, and the GHOSTS team: Resolving the Outer Disks and Halos of Nearby Galaxies . ...
... the existence of an unusual bar in the disk of NGC 1808 at a position angle of 155 ... axial ratio appears very large, whereas the bar-to-disk length ratio of about 0.3 is ...
... However, the dust extinction and confusion with stars in the disk of our Galaxy make this very difficult for ё25% of the sky, and the following questions remain unanswered: Could a nearby Andromedalike galaxy have escaped detection to date, hence change ...
[
Текст
]
Ссылки http://www.atnf.csiro.au/research/multibeam/papers/DeepSouth.ps.gz -- 482.5 Кб -- 07.04.1998 Похожие документы
... Disks Monday, November 03, 2014 Gas in the Periphery 8 :3 0 - 9 .0 0 9 :0 0 9 :1 0 ... Disk Periphery And Beyond Star Formation In The Extreme Outer Galaxy: Induced By HVC ...
[
Текст
]
Ссылки http://www.atnf.csiro.au/research/conferences/2014/ThePeripheryOfDisks/POD_Conference_Program_v5.pdf -- 102.5 Кб -- 11.11.2014 Похожие документы