Browse terms - alphabetical

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Term Definition Contributor Modified
Layout The structured arrangement of items in acollection. Ryan McGranaghan 2023.04.16
Lays No definition provided Christopher Rauch 2023.12.01
Lazarenkoite No definition provided Ryan McGranaghan 2023.04.16
Lazarettos No definition provided Christopher Rauch 2023.12.01
Lazulite No definition provided Ryan McGranaghan 2023.04.16
Lazurite No definition provided Ryan McGranaghan 2023.04.16
l band No definition provided Ryan McGranaghan 2023.04.16
LBHBand Lyman-Birge-Hopfield band in the farultraviolet range with wavelength range of 140nm to 170 nm. Ryan McGranaghan 2023.04.16
lbs No definition provided Ryan McGranaghan 2023.04.16
Lb variable stars No definition provided Ryan McGranaghan 2023.04.16
Lb variable stars No definition provided Ryan McGranaghan 2023.04.16
Lb variable stars No definition provided Ryan McGranaghan 2023.04.16
LCoordinateSystem No definition provided Ryan McGranaghan 2023.04.16
LCP Link checker periodicity describes the periodic verification of object links. Takes the value [integer](https://n2t.net/99152/h1210), which refers to the approximate number of times per year that the object is subject to automated link checking. Non-zero LCP related to [LCU](https://n2t.net/99152/h1230). Element may be updated. Sandra Sweat 2023.03.27
LCU Link checker uptime describes the outcome of object links. Takes the value [percentage](https://n2t.net/99152/h1216). Uptime, the availability of the link, should be expressed as a number from 0 to 10 0, for those objects with non-zero [LCP](https://n2t.net/99152/h1212), if known. Element may be updated. Sandra Sweat 2023.03.27
Lc variable stars No definition provided Ryan McGranaghan 2023.04.16
Lc variable stars No definition provided Ryan McGranaghan 2023.04.16
Lc variable stars No definition provided Ryan McGranaghan 2023.04.16
L dwarfs A type of brown dwarf with an effective temperature ranging from about 2200 K to about 1300 K, corresponding to luminosities about 4 x 10^-4 to 3 x 10^-5 times that of the Sun. L dwarfs are intermedia te in temperature between M and T dwarfs. Their spectra in the optical show weak titanium oxide (TiO) and vanadium oxide (VO) absorption lines and strong metallic hydrides CrH (8611 and 9969 Å) and FeH (8692 and 9896 Å). Also are present strong neutral atomic lines of alkali metals Na I (8183, 8195 Å), K I (7665, 7699 Å), Rb I (7800, 7948 Å), Cs I (8521, 8943 Å), and sometimes Li I (6708 Å). The prototype of the L-dwarf class is GD 165B. Ryan McGranaghan 2023.04.16
L dwarfs A type of brown dwarf with an effective temperature ranging from about 2200 K to about 1300 K, corresponding to luminosities about 4 x 10^-4 to 3 x 10^-5 times that of the Sun. L dwarfs are intermedia te in temperature between M and T dwarfs. Their spectra in the optical show weak titanium oxide (TiO) and vanadium oxide (VO) absorption lines and strong metallic hydrides CrH (8611 and 9969 Å) and FeH (8692 and 9896 Å). Also are present strong neutral atomic lines of alkali metals Na I (8183, 8195 Å), K I (7665, 7699 Å), Rb I (7800, 7948 Å), Cs I (8521, 8943 Å), and sometimes Li I (6708 Å). The prototype of the L-dwarf class is GD 165B. Ryan McGranaghan 2023.04.16
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