Astronomy and Astrophysics – Astronomy
Scientific paper
Nov 1998
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998apj...507l..83m&link_type=abstract
The Astrophysical Journal, Volume 507, Issue 1, pp. L83-L87.
Astronomy and Astrophysics
Astronomy
42
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.
Fukui Yasuo
Hara Atsushi
Hayakawa Takahiro
Kato Shigeo
Kawamura Akiko
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