


This system has an orbital period of 600 days and its SIMBAD spectral type is: M3ep+O D (hot "O-type") White dwarf.
I also took some LISA spectra from Mt. Pinos, CA (2500 meter elevation) in June and July (still processing my Aug18 spectra):


The He lines look like they're increasing (relative to balmer lines), but I need to confirm with my Aug18 LISA data.
James Foster
Los Angeles, CA