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- W2883131788 abstract "We have measured the relationships between HI mass, stellar mass and star formation rate using the HI Parkes All Sky-Survey Catalogue (HICAT) and the Wide-field Infrared Survey Explorer (WISE). Of the 3,513 HICAT sources, we find 3.4 micron counterparts for 2,896 sources (80%) and provide new WISE matched aperture photometry for these galaxies. For our principal sample of spiral galaxies with W1 $le$ 10 mag and z $le$ 0.01, we identify HI detections for 93% of the sample. We measure lower HI-stellar mass relationships that HI selected samples that do not include spiral galaxies with little HI gas. Our observations of the spiral sample show that HI mass increases with stellar mass with a power-law index 0.35; however, this value is dependent on T-type, which affects both the median and the dispersion of HI mass. We also observe an upper limit on the HI gas fraction, which is consistent with a halo spin parameter model. We measure the star formation efficiency of spiral galaxies to be constant 10$^{-9.57}$ yr$^{-1}$ $pm$ 0.4 dex for 2.5 orders of magnitude in stellar mass, despite the higher stellar mass spiral showing evidence of quenched star formation." @default.
- W2883131788 created "2018-08-03" @default.
- W2883131788 creator A5001267409 @default.
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- W2883131788 date "2018-08-29" @default.
- W2883131788 modified "2023-10-10" @default.
- W2883131788 title "Relationships between Hi Gas Mass, Stellar Mass, and the Star Formation Rate of HICAT+<i>WISE</i> (H i-<i>WISE</i>) Galaxies" @default.
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- W2883131788 doi "https://doi.org/10.3847/1538-4357/aad3b9" @default.
- W2883131788 hasPublicationYear "2018" @default.
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