Skip to main content
U.S. Department of Energy
Office of Scientific and Technical Information

CCD photometry of the sparse halo cluster E3

Journal Article · · Publ. Astron. Soc. Pac.; (United States)
DOI:https://doi.org/10.1086/131586· OSTI ID:5612863
New photometry in B and V for the sparse halo cluster E3 has been obtained with the prime-focus CCD camera at the CTIO 4-m telescope. The principal sequences are better defined than in the previous color-magnitude (C-M) diagrams, but the large scatter of evolved stars above the turnoff remains. The C-M morphology, inferred old age, and position in the halo definitely indicate that E3 is a globular cluster. Evidence for possible main-sequence binaries appears in the C-M diagram in the form of a sequence parallel to the cluster main sequence and three-quarters of a magnitude above it. The luminosity function drops off sharply, about 2.5 mag below the turnoff, supporting the suggestion by van den Bergh, Demers, and Kunkel (1980), that the cluster is severely truncated by tidal forces. 34 references.
Research Organization:
Dominion Astrophysical Observatory, Victoria, Canada
OSTI ID:
5612863
Journal Information:
Publ. Astron. Soc. Pac.; (United States), Journal Name: Publ. Astron. Soc. Pac.; (United States) Vol. 97; ISSN PASPA
Country of Publication:
United States
Language:
English

Similar Records

CCD photometry of the globular cluster Palomar 5
Journal Article · Mon Mar 31 23:00:00 EST 1986 · Astron. J.; (United States) · OSTI ID:6061289

Deep CCD photometry of the globular cluster NGC 7099
Journal Article · Sat Aug 01 00:00:00 EDT 1987 · Astrophys. J.; (United States) · OSTI ID:5839297

Deep CCD photometry in globular clusters. I. The Main sequence of M4
Journal Article · Tue Jan 31 23:00:00 EST 1984 · Astrophys. J.; (United States) · OSTI ID:6742199