Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 2007
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21113917s&link_type=abstract
American Astronomical Society, AAS Meeting #211, #139.17; Bulletin of the American Astronomical Society, Vol. 39, p.988
Astronomy and Astrophysics
Astronomy
Scientific paper
Recent observations of the tip of the Magellanic Stream with the Arecibo telescope have revealed very clumpy morphology of this gaseous tidal tail. We show that thermal instability, with a typical timescale of a few Myrs to a few hundreds of Myrs, can result in fragmentation of a warm tail of gas trailing through the Galactic Halo, and therefore naturally explain the formation of small, cool HI clouds. If the observed clumpiness at the tip of the Stream is primarily due to thermal instability, the characteristic size of thermal fragments allows us to place a limit on the age of the Magellanic Stream and the distance to its tip.
Douglas K.
Heiles Carl
Hoffman Silas
Peek J.
Putman Mary
No associations
LandOfFree
How Far Is The Tip Of The Magellanic Stream? 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 How Far Is The Tip Of The Magellanic Stream?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and How Far Is The Tip Of The Magellanic Stream? will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1482712