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

Part of: IAU Issue 315 - From Interstellar Clouds...

Published online by Cambridge University Press:  12 September 2016

Joana M. Oliveira ,
Jacco Th. van Loon  and
Marta Sewiło
Joana M. Oliveira
Affiliation:
Lennard-Jones Laboratories, School of Physical & Geographical Sciences, Keele University, UK
Jacco Th. van Loon
Affiliation:
Lennard-Jones Laboratories, School of Physical & Geographical Sciences, Keele University, UK
Marta Sewiło
Affiliation:
Space Science Institute & John Hopkins University, USA
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Abstract

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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.

Keywords

stars: formationHII regionsgalaxies: individual (LMC, SMC)
Type
Poster Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S315: From Interstellar Clouds to Star-Forming Galaxies: Universal Processes? , August 2015 , E61
Copyright
Copyright © International Astronomical Union 2016 

References

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