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Estimation of the Flux at 1450 MHz of OB Stars for FAST and SKA

  • Authors: Qichen Huang, 启宸 黄, Biwei Jiang, 碧沩 姜, Dingshan Deng, 丁山 邓, Bin Yu, 斌 于, Albert Zijlstra

Qichen Huang et al 2023 The Astronomical Journal 166 .

  • Provider: AAS Journals

Caption: Figure 2.

Comparison of T eff derived by Gaia/DR3 and LAMOST. The blue dot denotes the objects we filtered out by ﹩{({G}_{\mathrm{BP}}-{G}_{\mathrm{RP}})}_{0}\gt 0﹩ and ﹩{M}_{{{\rm{G}}}_{\mathrm{BP}}}\lt 2﹩. The yellow dot denotes the objects that pass photometry screening; however, T eff is lower than 12,500 K and therefore removed as well. The red dot denotes the stars for which we finally calculate the radio flux.

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