The Face-on View of the Milky Way: Gas Dynamics in the COBE NIR Bulge and Disk

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dc.creatorEnglmaier, Peter
dc.creatorGerhard, Ortwin E.
dc.date1998-12-08
dc.date.accessioned2026-07-07T02:29:33Z
dc.date.available2026-07-07T02:29:33Z
dc.descriptionWe report simulations of the gas flow in the gravitational potential of the COBE NIR bulge and disk. These models lead to four--armed spiral structure between corotation of the bar and the Sun, in agreement with the observed spiral arm tangents. The 3-kpc-arm is identified with one of the arms emanating from the ends of the bar.
dc.descriptionLatex, 4 pages, 2 figures. To appear in the proceedings of the `Galaxy Dynamics' conference held at Rutgers Univ., August 8-12, 1998
dc.identifierhttps://arxiv.org/abs/astro-ph/9812166
dc.identifierhttp://arxiv.org/abs/astro-ph/9812166
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13516
dc.subjectAstrophysics
dc.titleThe Face-on View of the Milky Way: Gas Dynamics in the COBE NIR Bulge and Disk
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