Herbig-Haro Objects, Bright, Variable Regions Within Nebulae, Are Now Thought

Herbig-Haro objects, bright, variable regions within nebulae, are now thought to be the result of:

A) the initial condensation of matter into a protostar, producing an infrared and visible glow.
B) intense jets of material ejected from a young star, hitting parts of the nebula.
C) brightening of the gas surrounding a massive star as the precursor to a supernova explosion.
D) the hot atmosphere of a star as it is ejected in the dying phases of the star's life.

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