Higher luminosity in stars directly correlates with increased power output, as luminosity is measured in energy per time, equivalent to watts. For example, a star that is ten times more luminous than another indeed emits ten times more power. The relationship holds true across varying luminosities, meaning a star that is 1,000 times more luminous would emit 1,000 times more power. White dwarfs, despite having high surface temperatures and radiation per square centimeter, exhibit lower total luminosity due to their smaller size. Thus, while luminosity and power are related, factors like size and temperature also influence a star's overall characteristics.