The Intermediate Velocity Cloud IVC86+38.5-45, Related to High Velocity Clouds?
1989 ◽
Vol 120
◽
pp. 458-458
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Examining the high velocity cloud complex C and its possible interaction with gas of the galactic disk we became aware of a dust cloud located at galactic longitude l = 86° and latitude b = 38°.5 seen in the l00µm image of the IRAS. This cloud consists of a cucumber shaped core surounded by a horseshoe shaped halo opening towards larger galactic coordinates. At very low 100µm intensities dust lanes starting at the core or the ends of the horseshoe can be traced for about 5° towards high galactic latitude and longitude.
1991 ◽
Vol 144
◽
pp. 93-96
1995 ◽
Vol 272
(3)
◽
pp. 599-604
◽
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