Variable Stars - Other types
Hills Observatory: 1 January 2013 to 10 June 2019
In addition to the six variable-star types described above, certain other symbols may be found in the Type data field: BLLAC  Extragalactic BL Lacertae-type objects. These are compact quasistellar        objects showing almost continuous spectra with weak emission and absorption        lines and relatively rapid irregular light changes with amplitudes up to 3 mag in        V or more. Sources of strong X-ray radiation and radio waves, their emission        displays strong and variable linear polarization in the visible and infrared spectral        regions. Some objects of this type, considered erroneously to be variable stars        and designated in the GCVS system, will probably sometimes be included in the        main table of the Catalogue in the future, too. CST  Nonvariable stars, formerly suspected to be variable and hastily designated.         Further observations have not confirmed their variability. GAL  Optically variable quasistellar extragalactic objects (active galactic nuclei         [AGNs]) considered to be variable stars by mistake.        L:     Unstudied variable stars with slow light changes. QSO  Optically variable quasistellar extragalactic sources (quasars) that earlier were         erroneously considered to be variable stars. S:    Unstudied variable stars with rapid light changes. *     Unique variable stars outside the range of the classifications described above.        These probably represent either short stages of transition from one variability        type to another or the earliest and latest evolutionary stages of these types,        or they are insufficiently studied members of future new types of variables.        +     If a variable star belongs to several types of light variability simultaneously, the        types are joined in the Type field by a "+" sign (e.g., E+UG, UV+BY).