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Molecular spiral structure in M51

Rand, R. J. and Kulkarni, S. R. (1990) Molecular spiral structure in M51. In: Submillimetre Astronomy. Astrophysics and Space Science Library. No.158. Springer Netherlands , Dordrecht, pp. 239-240. ISBN 9789401568524. https://resolver.caltech.edu/CaltechAUTHORS:20201117-175541343

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Abstract

We present a mosaic map of M51 in the ¹²CO 1→0 line made with the Owens Valley mm-interferometer. The molecular arms we see are narrow and show an offset relative to the Ha emission. They also show coincidence with the dust lanes. Several interarm emission regions have also been detected, but with very little accompanying Ha emission. We briefly discuss the evidence for density-wave triggering of star formation.


Item Type:Book Section
Related URLs:
URLURL TypeDescription
https://doi.org/10.1007/978-94-015-6850-0_91DOIArticle
https://rdcu.be/caZmbPublisherFree ReadCube access
ORCID:
AuthorORCID
Kulkarni, S. R.0000-0001-5390-8563
Additional Information:© Springer Science+Business Media Dordrecht 1990.
Subject Keywords:Density Wave, Star Form Region, Star Formation Process, Dust Lane, Wave Trigger
Series Name:Astrophysics and Space Science Library
Issue or Number:158
DOI:10.1007/978-94-015-6850-0_91
Record Number:CaltechAUTHORS:20201117-175541343
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20201117-175541343
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:106712
Collection:CaltechAUTHORS
Deposited By: Rebecca Minjarez
Deposited On:19 Nov 2020 16:30
Last Modified:16 Nov 2021 18:56

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