A slow-rotating white dwarf star can not exceed the Chandrasekhar limit of 1.44 solar masses without collapsing to form a neutron star or exploding as a Type Ia supernova.
rotation | Stellar classification | Earth's rotation | Stellar Kart | Rotation | crop rotation | Wick rotation | Summer's Stellar Gaze | Stellar collision | Rotation (music) | Crop rotation | Stellar wind (code name) | Stellar Wind | stellar wind | Stellar's Sea Eagle | Stellar Classification | stellar classification | Stellar atmosphere | Rotation matrix | Rotation (mathematics) | Rotation (album) | International Earth Rotation and Reference Systems Service | Hypercompact stellar system | Carrington rotation |