A kinematic analysis of the giant molecular complex W3: Possible evidence for cloud–cloud collisions that triggered OB star clusters in W3 Main and W3(OH)
W3 is one of the most outstanding regions of high-mass star formation in the outer solar circle, and includes two active star-forming clouds: W3 Main and W3(OH). Based on a new analysis of the ${^{12}\text{CO}(J = 2-1)}$ data obtained at $38^{\prime \prime }$ resolution, we have found three clouds t...
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| Published in: | Publications of the Astronomical Society of Japan 2024-10, Vol.76 (5), p.895-911 |
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| Main Authors: | , , , , , , , , |
| Format: | Article |
| Language: | English |
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| Online Access: | Get full text |
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