Abstract
The population of young stars associated with intermediate mass stars has been investigated in a sample of 19 Herbig AE/BE (HAEBE) stars. Based on star counts in the K band, we find that the presence of groups/clusters (at a level of 200-400 star pc-2) is observed only in association with stars of early B-types (<B7) and that the transition to the isolated mode of star formation is quite sharp.
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Lisi, F., Baffa, C., Bonaccini, D., Del Vecchio, C., Gennari, S., Hunt, L. K., Marcucci, G., & Stanga, R. 1996, PASP, 108, 364
Hillenbrand, L. A. 1995, PhD Thesis, University of Masachusetts
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© 1997 Springer Science+Business Media Dordrecht
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Testi, L., Maltagliati, S., Palla, F., Natta, A., Prusti, T. (1997). Clustering around Herbig AE/BE Stars. In: Garzón, F., Epchtein, N., Omont, A., Burton, B., Persi, P. (eds) The Impact of Large Scale Near-IR Sky Surveys. Astrophysics and Space Science Library, vol 210. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5784-1_34
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DOI: https://doi.org/10.1007/978-94-011-5784-1_34
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