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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

Cormier, D. et al. 2015, A&A, 578, 53 Google Scholar
Kaufman, M.J. et al. 1999, ApJ, 527, 795 CrossRefGoogle Scholar
Malhotra, S. et al. 2001, ApJ, 561, 766 CrossRefGoogle Scholar
Oliveira, J.M. et al. 2013, MNRAS, 428, 3001 CrossRefGoogle Scholar
Seale, J.P. et al. 2009, ApJ, 699, 150 Google Scholar
van Loon, J.Th. et al. 2010, AJ, 139, 1553 Google Scholar