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dc.contributor.authorBrinks, E.
dc.contributor.authorBigiel, Frank
dc.contributor.authorLeroy, Adam
dc.contributor.authorWalter, Fabian
dc.contributor.authorde Blok, W. J. G.
dc.contributor.authorBagetakos, Ioannis
dc.contributor.authorUsero, Antonio
dc.contributor.authorKennicutt, Robert C.
dc.contributor.editorAndersen, J.
dc.contributor.editorBland-Hawthorn, J.
dc.contributor.editorNordstrom, B.
dc.date.accessioned2011-11-24T15:01:08Z
dc.date.available2011-11-24T15:01:08Z
dc.date.issued2009
dc.identifier.citationBrinks , E , Bigiel , F , Leroy , A , Walter , F , de Blok , W J G , Bagetakos , I , Usero , A & Kennicutt , R C 2009 , H I in galactic disks . in J Andersen , J Bland-Hawthorn & B Nordstrom (eds) , Proceedings of the 24th Symposium of the IAU : Galaxy Disk in Cosmological Context . 1st edn , vol. 4 , Cambridge University Press , Cambridge , pp. 301-306 . https://doi.org/10.1017/S1743921308027725
dc.identifier.isbn978-0-521-88985-8
dc.identifier.otherPURE: 459824
dc.identifier.otherPURE UUID: 6edcff67-22c9-4965-885a-1395c90e3185
dc.identifier.otherWOS: 000264868200039
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407840
dc.identifier.urihttp://hdl.handle.net/2299/7131
dc.descriptionOriginal article can be found at: http://journals.cambridge.org/ Copyright International Astronomical Union
dc.description.abstractStudies of the atomic phase of the interstellar medium, via the 21-cm spectral line of neutral hydrogen (H I), play a key role in our attempts to understand the structure and evolution of disk galaxies. We present here results from The H I Nearby Galaxy Survey (THINGS) and focus on the mass distribution as derived from the observed kinematics, and on the link between gas and star formation rate surface density, i.e., the Schmidt-Kennicutt law. Also, we briefly dwell on the wealth and wide variety of structures'. often outlining what seem to be expanding shells surrounding sites of recent, massive star formation.en
dc.format.extent6
dc.language.isoeng
dc.publisherCambridge University Press
dc.relation.ispartofProceedings of the 24th Symposium of the IAU
dc.subjectgalaxies: structure
dc.subjectgalaxies: spiral
dc.subjectgalaxies: ISM
dc.titleH I in galactic disksen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1017/S1743921308027725
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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