Observations of the brightest globular clusters associated with NGC 5128

Details Observations of the brightest globular clusters associated with NGC 5128 Observations of the brightest globular clusters associated with NGC 5128

Jan 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981aj.....86...24v&link_type=abstract

Astronomical Journal, vol. 86, Jan. 1981, p. 24-29. Research supported by the Natural Sciences and Engineering Research Council

Astronomy and Astrophysics

Astronomy

31

Astronomical Photography, Astronomical Spectroscopy, Globular Clusters, Astronomical Catalogs, Brightness, Metals, Photographic Plates

Scientific paper

Six slightly nonstellar objects with V equal to or greater than 17.2 and image morphology similar to that of the globular cluster of Graham and Phillips (1980) have been found near NGC 5128 on CTIO 4-m prime focus plates. The coordinates of the six objects have been derived with an accuracy of 10 arcsec by comparison with the positions of the four SAO stars in the field. The location of the new six cluster suspects near NGC 5128 and radial velocity observations support the conclusion that their association with this galaxy is probably real.

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