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Statistical results from a jcmt survey of MM and sub-MM emission in herbig ae/be stars
Authors:S Skinner  A Brown  W Dent
Institution:(1) Inst. of Space & Astronautical Science, 3-1-1 Yoshinodai, 229 Sagamihara, Japan;(2) JILA / Univ. of Colorado, 80309-0440 Boulder, Co, USA;(3) Joint Astronomy Center, 660 N. Aohoku Pl., 96720 Hilo, HI, USA
Abstract:We have detected 1.1 mm continuum emission from 24 of 53 Herbig Ae/Be stars surveyed with the JCMT. Survival analysis shows that 1.1 mm luminosity is correlated with bolometric luminosity and with IRAS 25µm luminosity. For those stars that were also detected at 0.45 or 0.8 mm we find a typical flux dependence of the form S #x03BD; agrngr 3, which is steeper than that of most classical T Tauri stars.
Keywords:radio continuum: stars  stars: emission line  Be  stars: pre-main-sequence
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