Bibcode
DOI
Rosenberg, A.; Piotto, G.; Carraro, G.; Seleznev, A. F.
Referencia bibliográfica
Astronomy Reports, Volume 44, Issue 1, January 2000, pp.12-17
Fecha de publicación:
1
2000
Revista
Número de citas
7
Número de citas referidas
6
Descripción
The luminosity function of the globular cluster Palomar 1 is determined
together with its confidence interval by applying an adaptive kernel
estimator to data from the Isaac Newton Telescope. The luminosity
function of Palomar 1 has two minima in the V band and one in the I
band. The cluster core contains a relatively high fraction of bright
stars, indicative of mass segregation.