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Young Stellar Objects in the Magellanic Clouds: Herschel Spectroscopy First Results
Published online by Cambridge University Press: 12 September 2016
Abstract
We present preliminary results from spectroscopy obtained with PACS and SPIRE onboard the Herschel Space Observatory of a sample of massive Young Stellar Objects in the Magellanic Clouds. We analyse key gas-phase cooling species (Oi], [Cii], H2O, CO, OH), in order to characterise the physical conditions in these metal-poor environments.
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- Copyright © International Astronomical Union 2016