The Baryonic Tully-Fisher Relation. II.

We present new color-U (mass-to-light ratio) models to convert Wide-field Infrared Survey Explorer W1 fluxes into stellar masses. We outline a range of possible star formation...我们提出了全新的色U（质光比，mass-to-light ratio）模型，用于将广域红外巡天探测器（Wide-field Infrared Survey Explorer，简称WISE）的W1波段辐射通量转换为恒星质量。我们阐述了一系列可能的恒星形成