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The Extinction and Distance of the MBM Molecular Clouds at High Galactic Latitude

  • Authors: Mingxu Sun, Biwei Jiang, He Zhao, and Yi Ren

2021 The Astrophysical Journal Supplement Series 256 46.

  • Provider: AAS Journals

Caption: Figure 14.

The change of Teff (upper panel) and color excess ratios ﹩{E}_{\mathrm{NUV},{{\rm{G}}}_{\mathrm{BP}}}﹩/﹩{E}_{{{\rm{G}}}_{\mathrm{BP}},{{\rm{G}}}_{\mathrm{RP}}}﹩ (lower panel) with ﹩{\rm{\Delta }}{E}_{{{\rm{G}}}_{\mathrm{BP}},{{\rm{G}}}_{\mathrm{RP}}}^{\mathrm{MC}}﹩. Red asterisks are the results of the studied molecular clouds, while the blue asterisks are the simulation results considering the effective wavelength shift because of Teff and ﹩{\rm{\Delta }}{E}_{{{\rm{G}}}_{\mathrm{BP}},{{\rm{G}}}_{\mathrm{RP}}}^{\mathrm{MC}}﹩ (see Paper I for details).

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