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Survey of Oxygen-rich AGB Stars Using the KVN 4 Receiving Bands—SMASTES. I.

  • Authors: Hyeon Baek, Se-Hyung Cho, Jaeheon Kim, Seung-Min Son, Dong-Hwan Yoon, Kyung-Won Suh

Hyeon Baek et al 2025 The Astronomical Journal 170 .

  • Provider: AAS Journals

Caption: Figure 9.

IRAS two-color diagram of observational results for the P.F values of SiO21 and SiO11 masers according to the SRs, Miras, and OH/IR stars. Sources with a higher P.F value for SiO11 than SiO21 are marked in green, while those with a higher P.F value for SiO21 are marked in red. SiO21-only sources are identified in black with numbers (V Leo (#47) and OH43.8+0.5 (#112)). The curved and blue dashed lines represent the same as in Figure 8.

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