A ^13CO (J = 1-0) Search for Small Molecular Clouds toward the Chamaeleon-Musca Dark Cloud Complex

Astronomy and Astrophysics – Astronomy

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Ism: Clouds, Ism: Molecules, Ism: Individual: Name: Chamaeleon-Musca Dark Cloud Compex, Stars: Formation

Scientific paper

We have completed a ^13CO (J=1-0) survey for molecular clouds toward the Chamaeleon-Musca Dark Cloud Complex, covering an ~16^degx17^deg area with the NANTEN millimeter-wave telescope. The major result is a discovery of 25 small dense clouds widely distributed over ~11^degx13^deg (~28x33 pc at ~140 pc), in addition to the four previously known large dark clouds. The small clouds show a good spatial correlation with the 33 isolated X-ray-emitting T Tauri stars (TTSs), and most (~70%) of the 33 TTSs located within 4 pc of the small clouds' boundaries are likely formed in the small clouds. It is argued that the average density, >~10^3 cm^-3, and mass, ~20 M_solar, of the small clouds are large enough to form stars in them. The apparent lack of the associated molecular gas for the remaining TTSs is plausibly explained as a result of cloud dissipation due to the outflow activity of the X-ray TTSs. Based on the present findings, we conclude that the X-ray TTSs were formed in the small dense clouds and that it is not necessary to invoke a runaway TTS hypothesis.

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