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Infrared spectroscopy in the C–H stretching region towards embedded high-mass young stellar objects in the Large Magellanic Cloud

Published online by Cambridge University Press:  18 July 2017

Takashi Shimonishi ,
Emmanuel Dartois ,
Takashi Onaka  and
François Boulanger
Takashi Shimonishi
Affiliation:
Frontier Research Institute for Interdisciplinary Sciences, Tohoku University, Aramakiazaaoba 6-3, Aoba-ku, Sendai, Miyagi, 980-8578, Japan, email: [email protected]
Emmanuel Dartois
Affiliation:
Institut d'Astrophysique Spatiale, UMR 8617, Université Paris-Sud, bâtiment 121, 91405 Orsay, France
Takashi Onaka
Affiliation:
Department of Astronomy, Graduate School of Science, The University of Tokyo, 7-3-1 Hongo, Bunkyo-ku, Tokyo 113-0033, Japan
François Boulanger
Affiliation:
Institut d'Astrophysique Spatiale, UMR 8617, Université Paris-Sud, bâtiment 121, 91405 Orsay, France
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Abstract

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We report the results of infrared spectroscopic observations of embedded high-mass young stellar objects in the Large Magellanic Cloud. The CH3OH ice absorption band as well as the 3.47 μm absorption band are detected toward the embedded sources in the LMC. The properties of these spectral bands in the low metallicity environment are investigated based on comparisons with Galactic embedded sources.

Keywords

astrochemistryISM: abundancesISM: moleculesinfrared: ISMMagellanic Clouds
Type
Addendum
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29A: Astronomy in Focus , August 2015 , E27
Copyright
Copyright © International Astronomical Union 2017 

References

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