What key spectral feature distinguishes a Type II supernova progenitor, according to classification tables?
Presence of Hydrogen Lines
The initial classification system for supernovae relies heavily on the presence or absence of specific elemental signatures in the observed light spectrum. Type II supernovae are specifically characterized by the clear presence of Hydrogen Lines. This spectral signature indicates that the progenitor star, which undergoes core collapse, retained its outermost hydrogen envelope right up until the moment of explosion. This contrasts sharply with Type I supernovae, which, by definition, lack hydrogen lines. For instance, Type Ia events lack hydrogen and show strong ionized silicon, while Type Ib events lack hydrogen but show neutral helium lines, thus the defining feature for Type II is the intact hydrogen envelope evidenced by its spectral lines.
