The nature of the most distant M31 globular cluster candidate

Details The nature of the most distant M31 globular cluster candidate The nature of the most distant M31 globular cluster candidate

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26a...205....6b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 205, no. 1-2, Oct. 1988, p. 6-8. CNR-MPI-supported research.

Astronomy and Astrophysics

Astrophysics

6

Andromeda Galaxy, Astronomical Photography, Galactic Mass, Galactic Nuclei, Globular Clusters, Astronomical Photometry, Cross Correlation, Milky Way Galaxy, Radial Velocity

Scientific paper

CCD observations of the most distant M31 globular cluster candidate, vdB, have been obtained with the 152-cm Loiano telescope and with the intensified image dissector scanner at the KPNO 4-m telescope. The results indicate that this objects consists of two blended stars. It is suggested that vdB is not a M31 globular cluster, and that it should be disregarded in the analysis of M31 halo properties.

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