Ellipticity of five globular clusters in M31

Details Ellipticity of five globular clusters in M31 Ellipticity of five globular clusters in M31

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984pazh...10..275s&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 10, Apr. 1984, p. 275-278) Soviet Astronomy Letters (ISSN 0360-0327), vol. 10, Mar.-Apr

Astronomy and Astrophysics

Astronomy

Andromeda Galaxy, Astronomical Photography, Globular Clusters, Astronomical Maps, Ellipticity, Milky Way Galaxy, Photographic Plates

Scientific paper

A B-plate taken with the 2-m Ritchey-Chretien telescope of the Rozhen Observatory in Bulgaria has been processed by photographic isodensitometry to yield the ellipticity epsilon and major-axis position angle of five globular clusters in the Andromeda Nebula. These preliminary results suggest that the clusters in M31 have about the same flattening (epsilon = 0.05-0.16) as those in the Galaxy. Diameters estimated from the outer isodent apparently include the cluster coronae.

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