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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 03441naa a2200469 4500 | |
| 001 | oai:DiVA.org:kth-284415 | |
| 003 | SwePub | |
| 008 | 201105s2020 | |||||||||||000 ||eng| | |
| 009 | oai:DiVA.org:su-187712 | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-2844152 URI |
| 024 | 7 | a https://doi.org/10.1093/mnras/staa17952 DOI |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1877122 URI |
| 040 | a (SwePub)kthd (SwePub)su | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Brandenburg, Axelu Stockholms universitet,KTH,Nordic Institute for Theoretical Physics NORDITA,Stockholm Univ, Roslagstullsbacken 23, SE-10691 Stockholm, Sweden.;Stockholm Univ, Dept Astron, AlbaNova Univ Ctr, SE-10691 Stockholm, Sweden.;Univ Colorado, JILA, Boulder, CO 80303 USA.;Univ Colorado, Lab Atmospher & Space Phys, Boulder, CO 80303 USA.;Carnegie Mellon Univ, McWilliams Ctr Cosmol, Pittsburgh, PA 15213 USA.;Carnegie Mellon Univ, Dept Phys, Pittsburgh, PA 15213 USA.,Nordiska institutet för teoretisk fysik (Nordita),Institutionen för astronomi,University of Colorado, USA; Carnegie Mellon University, USA4 aut0 (Swepub:su)brandenb |
| 245 | 1 0 | a Application of a helicity proxy to edge-on galaxies |
| 264 | c 2020-06-29 | |
| 264 | 1 | b Oxford University Press,c 2020 |
| 338 | a print2 rdacarrier | |
| 500 | a QC 20201105 | |
| 520 | a We study the prospects of detecting magnetic helicity in galaxies by observing the dust polarization of the edge-on galaxy NGC 891. Our numerical results of mean-field dynamo calculations show that there should be a large-scale component of the rotationally invariant parity-odd B polarization that we predict to be negative in the first and third quadrants, and positive in the second and fourth quadrants. The large-scale parity-even E polarization is predicted to be negative near the axis and positive further away in the outskirts. These properties are shown to be mostly a consequence of the magnetic field being azimuthal and the polarized intensity being maximum at the centre of the galaxy and are not a signature of magnetic helicity. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 650 | 7 | a NATURVETENSKAPx Fysik0 (SwePub)1032 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciences0 (SwePub)1032 hsv//eng |
| 653 | a dynamo | |
| 653 | a MHD | |
| 653 | a polarization | |
| 653 | a turbulence | |
| 653 | a galaxies: individual: NGC 891 | |
| 653 | a galaxies: magnetic fields | |
| 700 | 1 | a Furuya, Ray S.u Tokushima Univ, Inst Liberal Arts & Sci, Minami Jousanajima Machi 1-1, Tokushima 7708502, Japan.4 aut |
| 710 | 2 | a KTHb Nordic Institute for Theoretical Physics NORDITA4 org |
| 773 | 0 | t Monthly notices of the Royal Astronomical Societyd : Oxford University Pressg 496:4, s. 4749-4759q 496:4<4749-4759x 0035-8711x 1365-2966 |
| 856 | 4 | u https://academic.oup.com/mnras/article-pdf/496/4/4749/33503899/staa1795.pdf |
| 856 | 4 | u https://doi.org/10.1093/mnras/staa1795y Fulltext |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:kth:diva-284415 |
| 856 | 4 8 | u https://doi.org/10.1093/mnras/staa1795 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-187712 |
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