High-resolution from Muana Kea - Surface photometry of galaxies in CL 0024 + 16

Details High-resolution from Muana Kea - Surface photometry of galaxies in CL 0024 + 16 High-resolution from Muana Kea - Surface photometry of galaxies in CL 0024 + 16

Jan 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986apj...300..639t&link_type=abstract

Astrophysical Journal, Part 1 (ISSN 0004-637X), vol. 300, Jan. 15, 1986, p. 639-657.

Other

26

Astronomical Photometry, Galactic Clusters, Galactic Structure, Brightness, Calibrating, Charge Coupled Devices, Elliptical Galaxies, Error Analysis, High Resolution

Scientific paper

A deep CCD image with resolution 0.6 arcsec FWHM has been obtained of the rich and distant galaxy cluster CL 0024 + 16 at z = 0.394. Even though most of the galaxies have major diameters less than 5 arcsec, the excellent image quality of the CCD frame and careful model fitting make it possible to determine the bulge and disk photometric characteristics for 26 galaxies. The nine blue 'Butcher-Oemler' galaxies in the field of view show a wide diversity of a structure: one is an elliptical, one a small bulge spiral, and the other seven have moderate to large bulge-to-disk ratios. The general morphology of the core of CL 0024 + 16 is also discussed.

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