Morphological analysis of spirals in the near-infrared.

Details Morphological analysis of spirals in the near-infrared. Morphological analysis of spirals in the near-infrared.

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996crasb.323..787h&link_type=abstract

Comptes Rendus de l'Academie des Sciences, Sér. II, Fasc. b, Tome 323, No. 11, p. 787 - 794

Computer Science

Spiral Galaxies: Morphology, Spiral Galaxies: Infrared Photometry

Scientific paper

Near-infrared images are used to study the morphology and the dust properties of three spiral galaxies: 1) ESO 320-26 exhibits a circumnuclear ring whose colours may be interpreted by the presence of dust and/or an active star-forming region. 2) In NGC 4219, the dust follows the inner ridge of the spiral arms and its bulge is partially obscured. 3) NGC 6810 has a very dissymmetric bulge, masked by dust and very red parts in the JHK plane corresponding to regions of highest extinction.

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