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|a 9781402025792
|9 978-1-4020-2579-2
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|a 10.1007/1-4020-2579-3
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|a High-Velocity Clouds
|h [electronic resource] /
|c edited by Hugo van Woerden, Bart Wakker, Ulrich Schwarz, Klaas de Boer.
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|a 1st ed. 2005.
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|a Dordrecht :
|b Springer Netherlands :
|b Imprint: Springer,
|c 2005.
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|a X, 406 p.
|b online resource.
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|a text
|b txt
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|a computer
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|a online resource
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|a text file
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|a Astrophysics and Space Science Library,
|x 2214-7985 ;
|v 312
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|a History of HVC research - an Overview -- HVC/IVC Maps and HVC Distribution Functions -- Kinematics of HV and IV Gas -- Interemdiate-velocity Clouds -- HVCS Related to the Magellanic System -- High-velocity Hi Gas in External Galaxies -- The Large- and Small-scale Structure of HVCs -- Ionized Gas Associated with HVCs -- The Coldest Phase in Halo High-velocity Gas: Dust and Molecules -- Distances and Metallicities of HVCS -- The Hot Halo -- HVCS Interacting With Their Environment -- Warps, Polar Rings and High-velocity Clouds -- High-Velocity Clouds: The Missing Link? -- Compact, Isolated High-velocity Clouds -- The Origin of the High-velocity Clouds -- Unsolved Mysteries of High-velocity Clouds.
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|a On the occasion of the retirement of Ulrich Schwarz, a symposium was held in Groningen in May of 1996, celebrating his contributions to the study of the int- stellar medium, including his work on the high-velocity clouds. The coming together of many specialists in the latter ?eld prompted the idea of compiling a book c- taining their contributions, and summarizing the status of our understanding of the high-velocity cloud phenomenon. This seemed especially worthwhile at the time, since many exciting developments were taking place. After the discovery of some H i clouds with high velocities, about 40 years ago, the subject had been dominated by 21-cm observations of H i emission. Starting in the mid-1980s much progress was being made because of the availability of new instruments, such as large ground-based optical telescopes and UV observatories in space. The connections between the work on high-velocity clouds and other studies of the properties of the (hot) interstellar medium also became clearer.
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|a Astronomy.
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|a Solar system.
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|a Astronomy, Cosmology and Space Sciences.
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|a Space Physics.
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|a van Woerden, Hugo.
|e editor.
|4 edt
|4 http://id.loc.gov/vocabulary/relators/edt
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|a Wakker, Bart.
|e editor.
|4 edt
|4 http://id.loc.gov/vocabulary/relators/edt
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|a Schwarz, Ulrich.
|e editor.
|4 edt
|4 http://id.loc.gov/vocabulary/relators/edt
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|a de Boer, Klaas.
|e editor.
|4 edt
|4 http://id.loc.gov/vocabulary/relators/edt
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|a SpringerLink (Online service)
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|t Springer Nature eBook
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|i Printed edition:
|z 9789048100811
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|i Printed edition:
|z 9789048166855
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|i Printed edition:
|z 9781402025785
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|a Astrophysics and Space Science Library,
|x 2214-7985 ;
|v 312
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|u https://doi.uam.elogim.com/10.1007/1-4020-2579-3
|z Texto Completo
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|a ZDB-2-PHA
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|a ZDB-2-SXP
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|a Physics and Astronomy (SpringerNature-11651)
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|a Physics and Astronomy (R0) (SpringerNature-43715)
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