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Asymmetric, Variable Hα Line Profile in Planetary Mass Object SR 12 c

  • Authors: Jun Hashimoto, Yuhiko Aoyama, Michihiro Takami, Shinsuke Takasao

Jun Hashimoto et al 2026 The Astronomical Journal 172 .

  • Provider: AAS Journals

Caption: Figure 1.

Hα spectra of SR 12 c from five individual datasets. All spectra show blueshifted peaks and are asymmetric with respect to the systemic velocity of −6.8 ± 3.0 km s−1 (A. Santamaría-Miranda et al. 2018; see also Figure 2). While spectra #1 and #2 show peaks at approximately −30 km s−1, the subsequent spectra show peaks at approximately −10 km s−1. A difference of −20 km s−1 is significant. While the velocity resolution in our observations are 6.1–7.5 km s−1, the data were binned to a velocity resolution of 10.5 km s−1 to increase SNR. Unidentified systematic effects may be present at approximately −175 and +175 km s−1 (see Section 2). The error bars are shown only for the first spectrum for presentation purposes. The absolute flux is provided as a reference (see Section 2).

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