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- W3100791526 abstract "We take advantage of the Gaia data release 2 to present 275 and 1,774 ultraviolet luminous stars in the FUV and the NUV. These stars are 5$sigma$ exceeding the centers of the reference frame that is built with over one million UV stars in the log $g$ vs $T_textrm{eff}$ diagram. The Galactic extinction is corrected with the 3D dusty map. In order to limit the Lutz-Kelker effect to an insignificant level, we select the stars with the relative uncertainties of the luminosity less than 40% and the trigonometric parallaxes less than 20%. We cross-identified our sample with the catalogs of RR Lyr stars and possible white dwarf main-sequence binaries, and find they compose $sim$ 62% and $sim$ 16% of our sample in the FUV and NUV, respectively. This catalog provides a unique sample to study stellar activity, spectrally unresolved compact main-sequence binaries and variable stars." @default.
- W3100791526 created "2020-11-23" @default.
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- W3100791526 date "2018-12-01" @default.
- W3100791526 modified "2023-10-16" @default.
- W3100791526 title "<i>Gaia</i>calibrated UV luminous stars in LAMOST" @default.
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- W3100791526 doi "https://doi.org/10.1088/1674-4527/18/12/156" @default.
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