Other
Scientific paper
Dec 1954
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1954bott....2k...3p&link_type=abstract
Boletín de los Observatorios de Tonantzintla y Tacubaya Vol. 2 Num. 11, pp. 3-10 (1954) (http://www.astroscu.unam.mx/bott/)
Other
Stars: Luminosity Function, Mass Function, Ism: Dust, Extinction
Scientific paper
The percentage of stars to be observed in different magnitude interval has been calculated for two regions similar in all their characteristics: except that one is a closed one, and the other has a considerably larger absorption constant. Simplifying assumptions have been made to carry out the calculations for several combination of parameter space, such as the dispersion in absolute magnitude, absorption constant, etc. As a principal result it si found that when extending the observations to fainter magnitudes, the increase of the number of stars observed, is faster for the obscured region.
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