'Dust continuum' presentation slideshows

Star Formation in our Galaxy

520 views • 38 slides

High resolution (sub)millimetre studies of the chemistry of low-mass protostars

404 views • 27 slides

The anatomy of starburst galaxies: sub-arcsecond mid-infrared observations

285 views • 16 slides

Radio Science and PILOT

Radio Science and PILOT. Tony Wong ATNF/UNSW PILOT Workshop 26 March 2003. New Synergies. PILOT: 2m, 1-30 ? m (10-300 THz). Starlight, thermal dust continuum, recombination lines, excited H 2 , PAH features.

177 views • 6 slides

Dust Continuum

Dust Continuum. Intensity ? Column density ? Mass. Dust emission. 1.3 mm dust emission (Motte & Andre 2001). Simple case:. If ? <<1 and T d =constant , Dust Temperature T d and emissivity spectral index b can be solved!. Under Rayleigh-Jeans limit and ? <<1,.

199 views • 4 slides