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Star Formation in NGC 5194 (M51a). II. The Spatially Resolved Star Formation Law

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dc.contributor.authorKennicutt, Robert C
dc.contributor.authorCalzetti, Daniela
dc.contributor.authorWalter, Fabian
dc.contributor.authorHelou, George
dc.contributor.authorHollenbach, David J.
dc.contributor.authorArmus, Lee
dc.contributor.authorBendo, George J
dc.contributor.authorDale, Daniel A
dc.contributor.authorDraine, Bruce T
dc.contributor.authorEngelbracht, Charles W
dc.contributor.authorGordon, Karl D
dc.contributor.authorPrescott, Moire K. M.
dc.contributor.authorRegan, Michael W.
dc.contributor.authorThornley, Michele D
dc.contributor.authorBot, Caroline
dc.contributor.authorBrinks, Elias
dc.contributor.authorde Blok, Willem
dc.contributor.authorde Mello, Dulia
dc.contributor.authorMeyer, Martin
dc.contributor.authorMoustakas, John
dc.contributor.authorMurphy, Eric J
dc.contributor.authorSheth, Kartik
dc.contributor.authorSmith, John-David T
dc.date.accessioned2015-12-07T22:21:08Z
dc.date.issued2007
dc.date.updated2015-12-07T08:54:20Z
dc.description.abstractWe have studied the relationship between the star formation rate (SFR), surface density, and gas surface density in the spiral galaxy M51a (NGC 5194), using multiwavelength data obtained as part of the Spitzer Infrared Nearby Galaxies Survey (SINGS ). We
dc.identifier.issn0004-637X
dc.identifier.urihttp://hdl.handle.net/1885/19904
dc.publisherIOP Publishing
dc.sourceAstrophysical Journal, The
dc.subjectKeywords: Galaxies: evolution; Galaxies: individual (M51a, NGC 5194); Galaxies: ISM; H II regions; Infrared: galaxies; Stars: formation
dc.titleStar Formation in NGC 5194 (M51a). II. The Spatially Resolved Star Formation Law
dc.typeJournal article
local.bibliographicCitation.issue1
local.bibliographicCitation.lastpage348
local.bibliographicCitation.startpage333
local.contributor.affiliationKennicutt, Robert C , University of Cambridge
local.contributor.affiliationCalzetti, Daniela, Space Telescope Science Institute
local.contributor.affiliationWalter, Fabian, Max Planck Institute for Astronomy
local.contributor.affiliationHelou, George, California Institute of Technology
local.contributor.affiliationHollenbach, David J., NASA Ames Research Center
local.contributor.affiliationArmus, Lee, Spitzer Science Center, Caltech
local.contributor.affiliationBendo, George J, Imperial College London
local.contributor.affiliationDale, Daniel A, University of Wyoming
local.contributor.affiliationDraine, Bruce T, Princeton University
local.contributor.affiliationEngelbracht, Charles W, University of Arizona
local.contributor.affiliationGordon, Karl D, University of Arizona
local.contributor.affiliationPrescott, Moire K. M., University of Arizona
local.contributor.affiliationRegan, Michael W., Space Telescope Science Institute
local.contributor.affiliationThornley, Michele D, Bucknell University
local.contributor.affiliationBot, Caroline, Spitzer Science Center, Caltech
local.contributor.affiliationBrinks, Elias, University of Hertfordshire
local.contributor.affiliationde Blok, Willem, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationde Mello, Dulia, Goddard Space Flight Centre
local.contributor.affiliationMeyer, Martin, Space Telescope Science Institute
local.contributor.affiliationMoustakas, John, New York University
local.contributor.affiliationMurphy, Eric J, Yale University
local.contributor.affiliationSheth, Kartik, Spitzer Science Center, Caltech
local.contributor.affiliationSmith, John-David T, University of Arizona
local.contributor.authoruidde Blok, Willem, u4191932
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationu4193696xPUB10
local.identifier.citationvolume671
local.identifier.doi10.1086/522300
local.identifier.scopusID2-s2.0-40249085653
local.type.statusPublished Version

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