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The 64 pages that link to White dwarf, each with the reason it gives.

• Stellar black holeCompared with: White dwarfs are lower-mass stellar remnants that do not undergo the same terminal collapse.

• Canis MinorNarrower topic: Procyon B is a nearby example of the stellar-remnant class.

• Dumbbell NebulaRelated: The exposed remnant at the nebula’s center supplies the ultraviolet radiation that lights its gas.

• NGC 6302Related: The exposed remnant at the nebula’s center is evolving toward a white dwarf.

• SN 1572Broader topic: A white dwarf was the exploding star in the event’s Type Ia interpretation.

• SubdwarfCompared with: White dwarfs are faint because they are cooling remnants, unlike hydrogen-burning subdwarfs.

• Beehive ClusterBroader topic: White dwarfs in the cluster preserve evidence of stars that have already evolved beyond the main sequence.

• Black dwarfNarrower topic: A black dwarf is the hypothetical cooled endpoint of this remnant.

• Edwin E. SalpeterRelated: Salpeter’s work on stellar evolution helped connect a star’s initial mass to its possible remnant.

• Exotic starCompared with: Its lower density and electron-supported structure differ sharply from exotic compact-star proposals.

• Messier 4Related: A white dwarf orbits the cluster’s millisecond pulsar.

• NGC 7027Related: The central star is evolving toward the white-dwarf state as its surrounding shell disperses.

• SN 1972ERelated: A white dwarf is the star whose thermonuclear disruption produces a Type Ia event like SN 1972E.

• Timeline of the far futureBroader topic: The Sun is expected to end as a white dwarf after shedding its outer layers.