Statistical Results from a JCMT Survey of MM and sub-mm Emission in Herbig Ae/Be Stars

Details Statistical Results from a JCMT Survey of MM and sub-mm Emission in Herbig Ae/Be Stars Statistical Results from a JCMT Survey of MM and sub-mm Emission in Herbig Ae/Be Stars

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..555s&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 555-556

Astronomy and Astrophysics

Astrophysics

1

Radio Continuum: Stars, Stars: Emission Line, Be, Stars: Pre-Main-Sequence

Scientific paper

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; αν 3, which is steeper than that of most classical T Tauri stars.

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