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[1])which can result in carbon detonation. These objects name an O·D·E describing their electron degeneracy pressure that can be solved to obtain an upper bound on (-5[1])the size of these objects of one point four solar masses, the Chandrasekhar limit. (-5[1])For 10 points, name these low-mass stellar remnants, the ultimate fate of red (10[1])giant stars. ■END■ (10[2])