Resolving the continuum emission form disks around T Tauri stars

Details Resolving the continuum emission form disks around T Tauri stars Resolving the continuum emission form disks around T Tauri stars

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997abos.conf..283w&link_type=abstract

Conference Paper, Astronomical and Biochemical Origins and the Search for Life in the Universe, IAU Colloquium 161, Publisher: B

Astronomy and Astrophysics

Astronomy

T Tauri Stars, Stellar Spectra, Continuous Radiation, Emission Spectra, Protostars, Microwave Imagery, Binary Stars, Stellar Evolution

Scientific paper

We report recent observations at millimeter wavelengths in which we have been able to resolve the continuum emission from the protostars HLTau and L1551/IRS5. Baselines of over 1 km have been recently added to the BIMA array, enabling angular resolutions of better than 0.5 arcsec at 2.7-mm wavelength. Using this new resolution, we have been able to image the continuum from HLTau and L1551/IRSS, finding a disk of radius of the order of 100 AU for HLTau and a binary of about 45 AU separation for L1551/IRS5.

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