| The HⅠ Gas Fraction Scaling Relation of the Green Pea Galaxies |
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| 引用本文： | 刘思琦,罗阿理,张伟,张彦霞,孔啸,赵永恒.The HⅠ Gas Fraction Scaling Relation of the Green Pea Galaxies[J].天文和天体物理学研究(英文版),2023(6):58-66. |
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| 作者姓名： | 刘思琦 罗阿理 张伟 张彦霞 孔啸 赵永恒 |
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| 作者单位： | 1. CAS Key Laboratory of Optical Astronomy,National Astronomical Observatories;2. University of Chinese Academy of Sciences;3. College of Computer and Information Management & Institute for Astronomical Science, Dezhou University |
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| 基金项目： | supported by the National Natural Science Foundation of China (Nos.12273075 and 12090041);;support from the National Key R&D Program of China (No.2021YFA1600401, 2021YFA1600400);;the Guangxi Natural Science Foundation (No.2019GXNSFFA 245008); |
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| 摘 要： | Green Pea galaxies are compact galaxies with high star formation rates. However, limited samples of Green Pea galaxies have H I 21 cm measurements. Whether the H I gas fraction( fH I≡ MH I/M) of Green Pea galaxies follows the existing scaling relations between the fH Iand NUV-r color or linear combinations of color and other physical quantities needs checking. Using archival data of H I 21 cm observations, we investigate the scaling relation of the NUV-r color with the MH I/M
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