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- W1585156987 abstract "I review recent observations of molecular gas in the halo of the Milky Way and in the Magellanic Clouds. Far-ultraviolet absorption line studies of molecular hydrogen (H_2) with ORFEUS and FUSE have unveiled the presence of a diffuse molecular hydrogen component in intermediate- and high-velocity clouds in the Galactic halo. Although the number of measurements is still quite small, the data suggests that diffuse H_2 in the halo exists only in clouds that contain a sufficient amount of heavy elements and dust, on whose surface the H_2 formation proceeds most efficiently. The implications of these observations for our understanding of the Milky Way halo are discussed." @default.
- W1585156987 created "2016-06-24" @default.
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- W1585156987 date "2001-09-12" @default.
- W1585156987 modified "2023-09-27" @default.
- W1585156987 title "Molecular Gas in the Galactic Halo and Beyond" @default.
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- W1585156987 hasPublicationYear "2001" @default.
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