When a white dwarf accretes mass from a companion and exceeds the Chandrasekhar limit of about 1.4 solar masses, instead of collapsing to a neutron star, it explodes as a Type 1A supernova. The reason is that a white dwarf is formed of relatively light elements like carbon and oxygen, so there is still a lot of thermonuclear energy available from further fusion reactions. So when the star gets compressed further, these thermonuclear reactions ignite and the star explodes in a massive explosion. By contrast, when the core of a more massive star collapses to form a neutron star, the core is formed of heavier elements like iron. Since iron is at the peak of the nuclear binding energy curve, there is no more thermonuclear energy available from further fusion reactions.