Linked from

The 11 pages that link to T Tauri star, each with the reason it gives.

• ProtostarCompared with: It is a later young-star stage, typically after the main protostellar accretion phase.

• Herbig–Haro objectRelated: The first recognized example lies near T Tauri, linking the nebulae to youth.

• Stellar activityRelated: Strong magnetic fields, accretion, and rapid rotation make these young stars highly variable.

• Pre-main-sequence starBroader topic: This class provides a well-studied example of low-mass stars before the main sequence.

• Stellar magnetic fieldBroader topic: Its magnetic field channels accretion and drives energetic young-star activity.

• Hayashi trackBroader topic: Many T Tauri stars occupy the Hayashi-track phase of stellar evolution.

• Herbig Ae/Be starCompared with: T Tauri stars are the lower-mass counterparts of Herbig Ae/Be stars.

• TW HydraeNarrower topic: TW Hydrae is a nearby example of this pre-main-sequence stellar class.

• Young stellar objectBroader topic: It is a recognizable later young-star phase after the embedded protostar stage.

• Formation and evolution of the Solar SystemRelated: Its winds and radiation help constrain how long the Sun’s planet-forming disk lasted.

• Viktor AmbartsumianBroader topic: These young stars exemplified the active, evolving objects central to his research.