Chemistry of protosolar-like nebulae: The molecular content of the DM Tau and GG Tau disks.

Details Chemistry of protosolar-like nebulae: The molecular content of the DM Tau and GG Tau disks. Chemistry of protosolar-like nebulae: The molecular content of the DM Tau and GG Tau disks.

Jan 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997a%26a...317l..55d&link_type=abstract

Astronomy and Astrophysics, v.317, p.L55-L58

Astronomy and Astrophysics

Astrophysics

155

Stars: T Tauri, Binaries: Close, Circumstellar Matter, Pre-Main Sequence, Radio-Lines: Stars

Scientific paper

We report the detection of CN, HCN, HNC, CS, HCO^+^, C_2_H and H_2_CO (ortho and para) in the protoplanetary disks of DM Tau and GG Tau. For the first time organic molecules are observed in objects representative of the presolar nebula. These molecules are underabundant with respect to the standard dense clouds. The depletions in the "outer" disk of DM Tau (100

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