Fig. 4 from Detection of a Violent Line Profile Variation of the 28SiO v = 2, J = 3

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Detection of a Violent Line Profile Variation of the ²⁸SiO v = 2, J = 3–2 Maser Emission toward Orion KL IRc2

Authors: Se-Hyung Cho, Hyun-Soo Chung, Hyo-Ryoung Kim, Hyun-Goo Kim, and Duk-Gyoo Roh

Cho et al. 1999 The Astronomical Journal 117 1485.

Caption: Fig. 4.

Spectra of the ²⁸SiO v = 0, J = 2–1, ²⁹SiO v = 0, J = 3–2, and ³⁰SiO v = 0, J = 3–2 transitions, observed in 1995 February and March.