These objects’ surface-confined g-modes were numerically computed by Don Winget in a paper that confirmed the elemental stratification of these objects’ envelopes. ZZ Cetis (-5[1])are a class of these objects (15[1]-5[1])of D·A·V type. (15[1])Classical estimates imply that the mass of these objects is inversely proportional to their volume. Accretion onto these objects produces (*) cataclysmic variables, (10[3])which can result (10[1])in carbon (10[1])detonation. (10[2])These objects (10[1])name an O·D·E (-5[2])describing their electron degeneracy (10[1])pressure (10[2]-5[1])that (10[1])can be solved (10[1]-5[1])to obtain an (10[1])upper bound on (-5[1])the size (10[3])of these objects (10[3])of (10[1])one point four (10[1]-5[1])solar masses, (10[1]-5[2])the (10[1])Chandrasekhar (10[1])limit. (10[1]-5[1])For 10 points, name these low-mass stellar remnants, the ultimate fate of red (10[1])giant stars. (10[4])■END■ (10[5]0[3])