On account of its inherent ambiguity (and the resulting inconsistency of its application) and negative associations, it is a label which it is hardly possible or useful to terminize.

However, the approximate locations of the Hayashi limits point to remarkably low masses for the three T Tauri stars investigated here. It should be noted, that the Hayashi limits are valid only for stars in hydrostatic equilibrium.

In his business ventures, he always looks after numero uno.

Thy virtue won me; with virtue preserve me.