Extra-planar H I in the Inner Milky Way

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

8 pages, 4 figures. Proceedings of the "Extra-planar Gas" conference, Dwingeloo, Netherlands, June 7-11, 2004. To appear in AS

Scientific paper

The extra-planar H I in the inner parts of the Milky Way has been discovered to contain numerous cloud-like structures when observed in the 21cm line with the Green Bank Telescope (GBT). These halo clouds have motions consistent with Galactic rotation and do not seem to be related to the classic high-velocity clouds. They are found to distances >1 kpc from the plane and can contain hundreds of solar masses of H I. Spectra of many of the halo clouds show evidence of coexisting cool and warm H I phases. A preliminary high-resolution study of one of the clouds suggests that it consists of a diffuse envelope and a few dense cores, with a peak H I column density reaching 4 x 10^20 cm^-2. The clouds are often organized into larger structures, one example of which was discovered near 35 degrees Galactic longitude rising higher than 2 kpc above the Galactic plane. New observations should answer some fundamental questions about the nature of these clouds.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Extra-planar H I in the Inner Milky Way 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 Extra-planar H I in the Inner Milky Way, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Extra-planar H I in the Inner Milky Way will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-169591

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.