We use the AllWISE Data Release to continue our search for WISE -detected motions .
In this paper , we publish another 27,846 motion objects , bringing the total number to 48,000 when objects found during our original AllWISE motion survey are included .
We use this list , along with the lists of confirmed WISE -based motion objects from the recent papers by Luhman and by Schneider et al .
and candidate motion objects from the recent paper by Gagné et al .
to search for widely separated , common-proper-motion systems .
We identify 1,039 such candidate systems .
All 48,000 objects are further analyzed using color-color and color-mag plots to provide possible characterizations prior to spectroscopic follow-up .
We present spectra of 172 of these , supplemented with new spectra of 23 comparison objects from the literature , and provide classifications and physical interpretations of interesting sources .
Highlights include : ( 1 ) the identification of three G/K dwarfs that can be used as standard candles to study clumpiness and grain size in nearby molecular clouds because these objects are currently moving behind the clouds , ( 2 ) the confirmation/discovery of several M , L , and T dwarfs and one white dwarf whose spectrophotometric distance estimates place them 5-20 pc from the Sun , ( 3 ) the suggestion that the Na i ‘ D ’ line be used as a diagnostic tool for interpreting and classifying metal-poor late-M and L dwarfs , ( 4 ) the recognition of a triple system including a carbon dwarf and late-M subdwarf , for which model fits of the late-M subdwarf ( giving [ Fe/H ] { \approx } - 1.0 ) provide a measured metallicity for the carbon star , and ( 5 ) a possible 24-pc-distant K5 dwarf + peculiar red L5 system with an apparent physical separation of 0.1 pc .