Linked from

The 14 pages that link to Herbig–Haro object, each with the reason it gives.

• Star formationBroader topic: These shock-brightened knots expose outflows launched during protostellar accretion.

• Molecular cloudBroader topic: These jets expose active star formation still embedded in cloud material.

• ProtostarBroader topic: These shock-brightened knots trace outflows from accreting protostars.

• Orion NebulaBroader topic: Jets from young stars in the nebula produce observable shock structures.

• T Tauri starBroader topic: These shock-brightened knots trace outflows from some accreting T Tauri systems.

• Bok globuleRelated: Such objects can signal outflows from young stars formed within or near globules.

• Cat's Eye NebulaCompared with: The nebula's fast knots resemble jet-driven shocks, but arise around an evolved star.

• Herbig Ae/Be starBroader topic: Some Herbig Ae/Be systems launch jets that produce these compact shock features.

• Rho Ophiuchi cloud complexBroader topic: Outflows from young stars can produce shock features in the complex's dense surroundings.

• Astrophysical jetBroader topic: These shock-brightened knots trace jets from forming stars.

• Circumstellar discRelated: Jets associated with accreting young stars trace processes linked to their discs.

• Trifid NebulaRelated: Such shock-brightened features trace outflows from young stars in star-forming regions like the Trifid.

• Young stellar objectBroader topic: These bright knots trace the outflows launched during active stellar formation.

• Viktor AmbartsumianBroader topic: Their energetic appearance connected with Ambartsumian’s emphasis on active processes in young stellar objects.