Observations of circumstellar disks at centimeter wavelengths

Details Observations of circumstellar disks at centimeter wavelengths Observations of circumstellar disks at centimeter wavelengths

Nov 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..106...11m&link_type=abstract

Icarus, vol. 106, p. 11

Physics

22

Stellar Envelopes, Centimeter Waves, Early Stars, T Tauri Stars, Submillimeter Waves, Very Large Array (Vla)

Scientific paper

A search for cm-wavelength dust emission from five embedded young stellar objects and three T Tauri stars has yielded emission from all of the former, but for only one of the latter, RY Tau. Standard circumstellar dust models for T Tauri dust emission allow the upper limits of the cm-wavelength fluxes of DL and GG Tau to constrain the properties of the circumstellar dust. Three of the five observed embedded sources showed ionized gas emission significantly stronger than any expected dust emission.

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