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

  • Takashi Shimonishi (a1), Emmanuel Dartois (a2), Takashi Onaka (a3) and François Boulanger (a2)

Abstract

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.

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References

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Allamandola, L. J., Sandford, S. A., Tielens, A. G. G. M., & Herbst, T. M., 1992, ApJ, 399, 134
Dartois, E., Schutte, W., Geballe, T. R., et al., 1999, A&A, 342, L32
Onaka, T., Matsuhara, H., Wada, T., et al., 2007, PASJ, 59, S401
Shimonishi, T., Onaka, T., Kato, D., et al., 2008, ApJ, 686, L99
Shimonishi, T., Onaka, T., Kato, D., et al. 2010, A&A, 514, A12
Shimonishi, T., Dartois, E., & Onaka, T., Boulanger, F., 2015, A&A, submitted
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Keywords

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

  • Takashi Shimonishi (a1), Emmanuel Dartois (a2), Takashi Onaka (a3) and François Boulanger (a2)

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