Infrared photometry of the globular cluster associated with NGC 5128

Details Infrared photometry of the globular cluster associated with NGC 5128 Infrared photometry of the globular cluster associated with NGC 5128

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980apj...241l..41f&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 241, Oct. 1, 1980, p. L41, L42.

Astronomy and Astrophysics

Astronomy

3

Astronomical Photometry, Galactic Clusters, Globular Clusters, Infrared Astronomy, Infrared Photometry, Hertzsprung-Russell Diagram, Peculiar Galaxies, Radio Galaxies

Scientific paper

Broad-band infrared photometry of a diffuse object discovered by Graham and Phillips in the vicinity of the peculiar galaxy NGC 5128 is presented. These data support their contention that this object is a moderately metal-rich globular cluster. At 2.2 microns its luminosity is comparable to, or as much as one magnitude brighter than, the brightest globulars observed in M31; the exact value depends on the distance modulus to NGC 5128.

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