Statistics – Computation
Scientific paper
Feb 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992apj...386l..47a&link_type=abstract
Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 386, Feb. 20, 1992, p. L47-L50. Research supported by Junta de An
Statistics
Computation
6
Milky Way Galaxy, Spatial Distribution, Star Formation, Wolf-Rayet Stars, Astronomical Catalogs, Computational Astrophysics, Density Distribution, Open Clusters
Scientific paper
Results are presented of a quantitative analysis of the sample of Wolf-Rayet stars with computed distances as listed in the catalog of Conti and Vacca (1990). Kernel methods are used to compute density distributions for the W-R stars, WN, and WC types, and the resulting structure is compared to the one depicted by the star-forming supercomplexes, as delineated by the population of young open clusters. A clear spatial link between both structures is shown.
Alfaro Emilio J.
Cabrera-Cano Jesus
Delgado Antonio J.
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