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dc.contributor.authorKrause, Martin
dc.contributor.authorDiehl, R.
dc.contributor.authorBagetakos, Y.
dc.contributor.authorBrinks, E.
dc.contributor.authorBurkert, A.
dc.contributor.authorGerhard, O.
dc.contributor.authorGreiner, J.
dc.contributor.authorKretschmer, K.
dc.contributor.authorSiegert, T.
dc.date.accessioned2015-07-20T07:51:35Z
dc.date.available2015-07-20T07:51:35Z
dc.date.issued2015-06-12
dc.identifier.citationKrause , M , Diehl , R , Bagetakos , Y , Brinks , E , Burkert , A , Gerhard , O , Greiner , J , Kretschmer , K & Siegert , T 2015 , ' 26 Al kinematics: superbubbles following the spiral arms? Constraints from the statistics of star clusters and HI supershells ' , Astronomy and Astrophysics , vol. 578 , A113 . https://doi.org/10.1051/0004-6361/201525847
dc.identifier.issn0004-6361
dc.identifier.otherBibtex: urn:67b2cf63815bd7c40a03bb98a3a7ad15
dc.identifier.otherORCID: /0000-0002-7758-9699/work/30407795
dc.identifier.otherORCID: /0000-0002-9610-5629/work/63687362
dc.identifier.urihttp://hdl.handle.net/2299/16182
dc.description.abstractHigh energy resolution spectroscopy of the 1.8 MeV radioactive decay line of 26Al with the SPI instrument on board the INTEGRAL satellite has recently revealed that diffuse 26Al has large velocities in comparison to other components of the interstellar medium in the Milky Way. 26Al shows Galactic rotation in the same sense as the stars and other gas tracers, but reaches excess velocities up to 300 km s−1en
dc.format.extent6
dc.format.extent724476
dc.language.isoeng
dc.relation.ispartofAstronomy and Astrophysics
dc.subjectgamma rays: ISM, ISM: kinematics and dynamics, ISM: bubbles, ISM: structure, Galaxy: structure
dc.subjectAstronomy and Astrophysics
dc.title26Al kinematics: superbubbles following the spiral arms? : Constraints from the statistics of star clusters and HI supershellsen
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionSchool of Physics, Engineering & Computer Science
dc.contributor.institutionDepartment of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1051/0004-6361/201525847
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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