OBSERVATIONS OF SiO <i>J</i> = 3-2 AND <i>J</i> = 2-1 EMISSION IN LATE-TYPE STARS. II.
Se‐Hyung Cho(Korea Astronomy and Space Science Institute), Jaehoon Jung(Korea Astronomy and Space Science Institute), Hyo-Ryoung Kim(Yonsei University), Hyun‐Goo Kim(Korea Astronomy and Space Science Institute), Hyunsoo Chung(Seoul National University), Duk-Gyoo Roh(Korea Astronomy and Space Science Institute)
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