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What: |
Probing the formation of O stars |
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Who: |
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(Max Planck Institute for Radio Astronomy) |
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When: |
Friday morning, May 21th, 10:30 a.m |
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Where: |
Room 2402, Mengminwei Buliding, (NJU) |
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Welcome to attend |
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( PMO Academic committee & academic circulating committee) |
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abstract
Star formation is a fundamental problem in astrophysics. While there is a generally accepted picuture on how Sun-like stars form, massive star formation has long been a mystery, and the formation mechanism of most massive O stars are particularly highly debated. Here I will show high-angular-resolution dust continuum and molecular line observations of two O-star-forming regions, one in a very young, proto-stellar stage and the other in a relatively more developed stage, and discuss their implications on the underlying star-forming mechanism.
