Spectroscopic studies of extragalactic YSOs have shown a great progress in the last few years. Infrared observations with AKARI made significant contributions to that progress. In this proceeding, we are going to introduce our current research on the infrared observations of ices and dust around embedded YSOs in the Magellanic Clouds.

ABSTRACT
1. INTRODUCTION
2. EMBEDDED YSO SAMPLES IN THE MAGELLANIC CLOUDS
3. WHAT DO WE LEARN FROM MAGELLANIC YSOs?
    3.1. Infrared Luminosity vs. Ice Column Density Relation
    3.2. Effect of Metallicity on Circumstellar Ices
4. SPATIAL SCALE PROBED BY OBSERVATIONS OF MAGELLANIC YSOs
5. SUMMARY
REFERENCES

• H. KANEDA(Graduate School of Science, Nagoya University)
• A. KAWAMURA(National Astronomical Observatory of Japan)
• Y. ITA(Astronomical Institute, Graduate School of Science, Tohoku University)
• I. SAKON(Department of Astronomy, Graduate School of Science, The University of Tokyo)
• D. KATO(Center for Low Carbon Society Strategy, Japan Science and Technology Agency)
• T. ONAKA(Department of Astronomy, Graduate School of Science, The University of Tokyo)
• T. SHIMONISHI(Department of Earth and Planetary Sciences, Graduate School of Science, Kobe University, Research Fellow of the Japan Society for the Promotion of Science)