Observation of High Redshift Galaxies: A Quantitative Approach to Galaxy Morphology.

Details Observation of High Redshift Galaxies: A Quantitative Approach to Galaxy Morphology. Observation of High Redshift Galaxies: A Quantitative Approach to Galaxy Morphology.

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..277b&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

With the HST and ground-based large telescopes observations of high redshift galaxies, the observed rest-frame wavelength shifts to the ultraviolet range. The usual classification tools (Hubble sequence, Concentration, Asymmetry, etc.) are less and less informative. So, it clearly appears that we need to define new ways of classifying the galaxies that would be valid whatever the rest-frame observed wavelength.

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