dc.contributor.author | Laine, S. | |
dc.contributor.author | Knapen, J. | |
dc.contributor.author | Perez-Ramirez, D. | |
dc.contributor.author | Doyon, R. | |
dc.contributor.author | Nadeau, D. | |
dc.date.accessioned | 2009-07-22T12:50:23Z | |
dc.date.available | 2009-07-22T12:50:23Z | |
dc.date.issued | 2001 | |
dc.identifier.citation | Laine , S , Knapen , J , Perez-Ramirez , D , Doyon , R & Nadeau , D 2001 , ' Grand-design spirals in the core of NGC 5248 ' , Astrophysics and Space Science , vol. 276 , no. 2/4 , pp. 475-482 . https://doi.org/10.1023/A:1017576024087 | |
dc.identifier.issn | 0004-640X | |
dc.identifier.other | PURE: 156567 | |
dc.identifier.other | PURE UUID: 22843b0a-b204-4726-baa2-50b9ea428aba | |
dc.identifier.other | dspace: 2299/3700 | |
dc.identifier.other | Scopus: 0035647968 | |
dc.identifier.uri | http://hdl.handle.net/2299/3700 | |
dc.description | “The original publication is available at www.springerlink.com”. Copyright Springer. [Full text of this article is not available in the UHRA] | |
dc.description.abstract | We report the detection of a bisymmetric nuclear spiral structure in the spiral galaxy NGC 5248.The two red spiral arms can be followed for about 3 arcsec, before they appear to end inside the radius of the circumnuclear starburst `ring' at about 5.5 arcsec or 400 pc distance from the nucleus. We combine our near-infrared Canada–France–Hawaii Telescope adaptive optics images with traditional near-infrared and optical images and show that spiral structure is present in this galaxy at spatial scales reaching from a hundred parsecs to 15 kpc. Comparison with a Hubble Space Telescope ultraviolet image shows how the starburst ring is related to the nuclear spiral structure. We also show a two-dimensional Hα velocity field that reveals no evidence for systematic streaming motions near the nuclear spiral or the starburst ring, nor for a rapidly rising rotation curve. | en |
dc.language.iso | eng | |
dc.relation.ispartof | Astrophysics and Space Science | |
dc.title | Grand-design spirals in the core of NGC 5248 | en |
dc.contributor.institution | School of Physics, Astronomy and Mathematics | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | https://doi.org/10.1023/A:1017576024087 | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |