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Abstract

We produce a detailed map of the perturbed surface density of neutral hydrogen in the outer Milky Way disk, demonstrating that the Galaxy is a non-axisymmetric multiarmed spiral. Spiral structure in the southern half of the Galaxy can be traced out to at least 25 kiloparsecs, implying a minimum radius for the gas disk. Overdensities in the surface density are coincident with regions of reduced gas thickness. The ratio of the surface density to the local median surface density is relatively constant along an arm. Logarithmic spirals can be fit to the arms with pitch angles of 20° to 25°.

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We thank P. Kalberla for providing a copy of the LAB HI survey and J. Peek, C. Laver, and T. Robishaw for helpful advice regarding plots. E.S.L. and L.B. were supported by NSF grant AST 02-28963. C.H. was supported by NSF grant AST 04-06987.

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Science
Volume 312 | Issue 5781
23 June 2006

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Received: 7 April 2006
Accepted: 22 May 2006
Published in print: 23 June 2006

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Authors

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E. S. Levine* [email protected]
Astronomy Department, University of California, 601 Campbell Hall, Berkeley, CA 94720, USA.
Leo Blitz
Astronomy Department, University of California, 601 Campbell Hall, Berkeley, CA 94720, USA.
Carl Heiles
Astronomy Department, University of California, 601 Campbell Hall, Berkeley, CA 94720, USA.

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To whom correspondence should be addressed. E-mail: [email protected]

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