Clustering around Herbig AeBe stars

Details Clustering around Herbig AeBe stars Clustering around Herbig AeBe stars

Oct 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999mnras.309..461b&link_type=abstract

Monthly Notices, Volume 309, Issue 2, pp. 461-464.

Physics

33

Scientific paper

We show that the observed correlation between the luminosity of young stars and the richness of associated clusters does not necessarily imply that there is a physical mechanism that favours the formation of massive stars in clusters. Instead, the data are compatible with a scenario in which stars are assembled at random into clusters with a spectrum of membership number, N. We also show that the required spectrum is of the form g(N)~N-α, where α is in the range 1.5 to 2, and note that this is also the mass spectrum of clumps in molecular gas.

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