Young Stellar Objects in the Magellanic Clouds: Herschel Spectroscopy First Results

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 condit...

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Bibliographic Details
Published in:Proceedings of the International Astronomical Union 2015-08, Vol.11 (S315), p.1-2, Article E61
Main Authors: Oliveira, Joana M., van Loon, Jacco Th, Sewiło, Marta
Format: Article
Language:English
Subjects:
Astronomical bodies
Astronomy
Astrophysics
Clouds
Cooling
Magellanic clouds
Onboard
Poster Papers
Spectroscopy
Spectrum analysis
Spires
Star & galaxy formation
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Summary: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.
ISSN:1743-9213
1743-9221
DOI:10.1017/S1743921316008231