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HST/NICMOS Survey in the 30 Doradus Nebular Filaments
Published online by Cambridge University Press: 25 May 2016
Abstract
On the basis of ample evidence accumulated during recent years for current star formation within the 30 Doradus Nebula, which appears to have been triggered by the massive central cluster (R136) in and just beyond the curved nebular filaments surrounding it, an HST/NICMOS survey of these regions was undertaken.
- Type
- Part 3. Massive Stars and 30 Doradus
- Information
- Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 245 - 246
- Copyright
- Copyright © Astronomical Society of the Pacific 1999