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Hunting for Globular Cluster Candidates in the Far Halo (D > 20 kpc) of M 31 by the Tautenburg Schmidt Telescope

Published online by Cambridge University Press:  26 July 2016

L. Federici ,
F. Bonoli ,
F. Fusi Pecci ,
B. Marano ,
F. Börngen  and
H. Meusinger
L. Federici
Affiliation:
Osservatorio Astronomico, Bologna, Italy
F. Bonoli
Affiliation:
Dipartmento di Astronomia, Bologna, Italy
F. Fusi Pecci
Affiliation:
Osservatorio Astronomico, Bologna, Italy
B. Marano
Affiliation:
Osservatorio Astronomico, Bologna, Italy
F. Börngen
Affiliation:
Karl-Schwarzschild-Observatorium, Tautenburg, Germany
H. Meusinger
Affiliation:
Karl-Schwarzschild-Observatorium, Tautenburg, Germany

Extract

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The M 31 cluster system is the largest sample of globular clusters found in the Local Group, is sufficiently close to allow quite easy observations, and is negligibly affected by total reddening, at least for a large outer sub-set. Unfortunately, a complete and uncontaminated sample of M 31 clusters is not available yet for two basic reasons:

Type
Part Twelve: Properties of Nearby Galaxies
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 583 - 586
Copyright
Copyright © Kluwer 1994 

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