Cold dust around Chamaeleon stars

Details Cold dust around Chamaeleon stars Cold dust around Chamaeleon stars

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994ap%26ss.212..215h&link_type=abstract

Astrophysics and Space Science, vol. 212, nos. 1-2, p. 215-220

Astronomy and Astrophysics

Astrophysics

6

Cosmic Dust, Millimeter Waves, Star Formation, A Stars, B Stars, Molecular Clouds, Spectral Energy Distribution, Stellar Models, Thermal Radiation

Scientific paper

Here we present the results of 1.3 millimeter continuum measurements for intermediate-mass stars in the Chamaeleon system of dark clouds. The detected millimeter radiation is most probably thermal emission from cold circumstellar dust grains. The measured millimeter fluxes are combined with infrared observations to model the broad-band spectral energy distribution (SED). In this way the parameters of the emission regions are determined.

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