Detection of a Violent Line Profile Variation of the [TSUP]28[/TSUP]S[CLC]i[/CLC]O [CLC][ITAL]v[/ITAL][/CLC] = 2, [ITAL]J[/ITAL] = 3–2 Maser Emission toward Orion KL IR[CLC]c[/CLC]2

Se‐Hyung Cho(Korea Astronomy and Space Science Institute), Duk-Gyoo Roh(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)
The Astronomical Journal
March 1, 1999
Cited by 3


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