Astronomy and Astrophysics – Astrophysics
Scientific paper
2005-05-31
Astron.Astrophys. 423 (2004) 895-907
Astronomy and Astrophysics
Astrophysics
28 pages with 23 figures
Scientific paper
10.1051/0004-6361:20040177
From an analysis of the sky and velocity distributions of the high-velocity clouds (HVCs) we show that the majority of the HVCs has a common origin. We conclude that the HVCs surround the Galaxy, forming a metacloud of 300 kpc in size and with a mass of 3 10^9 M_sun, and that they are the product of a powerful ``superwind'' (about 10^58 ergs), which occurred in the Magellanic Clouds about 570 Myr ago as a consequence of the interaction of the Large and Small Magellanic Clouds. The HVCs might be magnetic bubbles of semi-ionized gas, blown from the Magellanic Clouds around 570 Myr ago, that circulate largely through the halo of the Galaxy as a stream or flow of gas.
No associations
LandOfFree
The high-velocity clouds and the Magellanic Clouds does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with The high-velocity clouds and the Magellanic Clouds, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The high-velocity clouds and the Magellanic Clouds will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-326489