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- W2980623897 abstract "While NGC 3603 is often quoted as the most massive visible Giant H ii Region in the Galaxy, there are other similar and even more massive regions now being found towards the inner Galaxy in the near-IR. Nevertheless, NGC 3603 still retains the status of clone to the dense core-object in 30 Dor, R 136 — but 7x closer and 49x less crowded! This paper summarizes the most recent findings concerning NGC 3603's color-magnitude diagram (CMD), initial mass function (IMF), mass segregation and stellar content — including its unusually luminous H-rich WNL members — down to its pre-main-sequence stars near the H-burning limit. Of special relevance are new high-resolution X-ray and radio images as related to merging/colliding winds and three massive proplyd-like objects. NGC 3603 is a somewhat younger, hotter, scaled-down version of typical starbursts found in other galaxies." @default.
- W2980623897 created "2019-10-25" @default.
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- W2980623897 date "2003-01-01" @default.
- W2980623897 modified "2023-09-30" @default.
- W2980623897 title "Galactic starburst NGC 3603 from X-rays to radio" @default.
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- W2980623897 doi "https://doi.org/10.1017/s0074180900212710" @default.
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