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| Name：Georgebex | 29, Nov, 2023 08:20:45 | |
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and there arranged. We use the stellar SEDs to estimate the spectral types of the three newly identified O stars in RCW49 and one previously undiscovered O star in M17. One of the bowshocks in RCW49 reveals the presence of a large scale flow of gas escaping the HII region. Radiation transfer modelin | |
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