arXiv:astro-ph/9911455AbstractReferencesReviewsResources
Discovery of molecular hydrogen in a high-velocity cloud of the Galactic halo
P. Richter, K. S. de Boer, H. Widmann, N. Kappelmann, W. Gringel, M. Grewing, J. Barnstedt
Published 1999-11-24Version 1
We report the discovery of molecular hydrogen absorption in a Galactic high-velocity cloud (HVC) in the direction of the Large Magellanic Cloud. For the same HVC we derive an iron abundance which is half of the solar value. Thus, all evidence points to a Galactic origin for high-velocity cloud complex in front of the LMC.
Comments: Published in Nature, this week; 14 pages, 3 figures
DOI: 10.1038/46492
Categories: astro-ph
Keywords: galactic halo, high-velocity cloud complex, molecular hydrogen absorption, large magellanic cloud, galactic high-velocity cloud
Tags: journal article
Related articles: Most relevant | Search more
Not enough stellar Mass Machos in the Galactic Halo
arXiv:astro-ph/9905240 (Published 1999-05-19)
UHECR Anisotropy and the Galactic Halo
arXiv:astro-ph/0307057 (Published 2003-07-02)
Formation of the Galactic Halo