Journal article

The gaseous haloes of disc galaxies

Abstract:: The study of gas outside the plane of disc galaxies is crucial to understanding the circulation of material within a galaxy and between galaxies and the intergalactic environment. We present new HI observations of the edge-on galaxy NGC891, which show an extended halo component lagging behind the disc in rotation. We compare these results for NGC891 with other detections of gaseous haloes. Finally, we present a dynamical model for the formation of extra-planar gas.

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APA Style

Fraternali, F., Oosterloo, T., Binney, J., & Sancisi, R. (2005). The gaseous haloes of disc galaxies.

MLA Style

Fraternali, F, et al. The Gaseous Haloes of Disc Galaxies. 2005.

Chicago Style

Fraternali, F, T Oosterloo, J Binney, and R Sancisi. 2005. The Gaseous Haloes of Disc Galaxies.
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Authors

+ Fraternali, F More by this author

Role:: Author

+ Oosterloo, T More by this author

Role:: Author

+ Binney, J More by this author

Institution:: University of Oxford
Division:: MPLS
Department:: Physics
Sub department:: Theoretical Physics
Role:: Author

+ Sancisi, R More by this author

Role:: Author

Publication date:: 2005-10-26

Keywords:: astro-ph
Pubs id:: pubs:167482
UUID:: uuid:da814517-e072-44d3-86a9-b59cacaed94d
Local pid:: pubs:167482
Source identifiers:: 167482
Deposit date:: 2013-02-20
ARK identifier:: ark:/29072/ora_da814517e07244d386a9b59cacaed94d

Terms of use

Copyright date:: 2005
Notes:: 6 pages, 2 figures; to appear in the proceedings of the Island
Universes conference held in Terschelling, Netherlands, July 2005, ed. R. de
Jong

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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