Photoelectric scanning of globular clusters. I - The inner structure of M3

Details Photoelectric scanning of globular clusters. I - The inner structure of M3 Photoelectric scanning of globular clusters. I - The inner structure of M3

Mar 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977mmsai..48...67b&link_type=abstract

Società Astronomica Italiana, Memorie, vol. 48, Mar. 1977, p. 67-76.

Astronomy and Astrophysics

Astronomy

5

Electrophotometry, Globular Clusters, Integral Equations, Optical Scanners, Density Wave Model, Luminous Intensity, Space Density, Stellar Magnitude, Volterra Equations

Scientific paper

By photoelectric scanning at constant speed, the integrated profile in V light of the central region of M3 down to a radius of 6 min is obtained. The integral equations relating the observed profile to the surface brightness and to the space light density are solved by a regularization method, which does not require the usual numerical filtering or a priori hypothesis on the analytical expression of the sought distributions. The behavior of the space light density thus obtained is consistent with the hypothesis (Kholopov 1953, 1955) on the existence of density waves in the space distribution of the most luminous stars.

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