Morphological Parameters of a Spitzer Survey of Stellar Structure in Galaxies

Autor: Sharon E. Meidt, Dennis Zaritsky, Jarkko Laine, S. Comeron, T. Mizusawa, Heikki Salo, Nor Pirzkal, J. H. Knapen, Benne W. Holwerda, Mark Seibert, J. L. Hinz, Michael W. Regan, Karín Menéndez-Delmestre, J. C. Muñoz-Mateos, Kartik Sheth, A. Gil-de-Paz, S. Erroz-Ferrer, A. Bosma, Seppo Laine, Eija Laurikainen, Dimitri A. Gadotti, Tae Jung Kim, Luis C. Ho, E. Athanassoula

Publikováno v: ASTROPHYSICAL JOURNAL
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
The Astrophysical Journal
The Astrophysical Journal, American Astronomical Society, 2014, 781 (1), ⟨10.1088/0004-637X/781/1/12⟩
E-Prints Complutense. Archivo Institucional de la UCM
instname
The Astrophysical Journal, 2014, 781 (1), ⟨10.1088/0004-637X/781/1/12⟩

International audience; The morphology of galaxies can be quantified to some degree using a set of scale-invariant parameters. Concentration (C), asymmetry (A), smoothness (S), the Gini index (G), the relative contribution of the brightest pixels to

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_dedup___::16b6464f2199279fdbd6c249398b8585
https://resolver.caltech.edu/CaltechAUTHORS:20140211-114726941