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 are a class of these objects of D·A·V type. Classical estimates imply that the mass of these objects is inversely proportional to their volume. Accretion onto these objects produces (*) cataclysmic variables, (10[2])which can result (10[1])in carbon detonation. (10[1])These objects name an O·D·E describing their electron degeneracy pressure (10[1]-5[1])that can be solved (10[1])to obtain an upper bound on the size (10[1])of these objects of one point four (10[1])solar masses, the Chandrasekhar limit. For 10 points, name these low-mass stellar remnants, the ultimate fate of red giant stars. ■END■ (10[1])