Herbig–Haro object

Summary

Herbig–Haro object is an astronomical object type^[1]. It draws 300 Wikipedia views per month (astronomical_object_type category, ranking #96 of 289).^[2]

Key Facts

• Herbig–Haro object's instance of is recorded as astronomical object type^[3].
• George Herbig is named after Herbig–Haro object^[4].
• Guillermo Haro is named after Herbig–Haro object^[5].
• Herbig–Haro object is a type of emission nebula^[6].
• Herbig–Haro object is part of galaxy^[7].
• Herbig–Haro object's Commons category is recorded as Herbig–Haro objects^[8].
• Herbig–Haro object's topic's main category is recorded as Category:Herbig–Haro objects^[9].
• Herbig–Haro object's different from is recorded as Herbig Ae/Be star^[10].

Body

Definition and Type

Herbig–Haro object's instance of is recorded as astronomical object type^[3]. It is a type of emission nebula^[6].

Origins

Things named after include George Herbig^[4], an astronomer^[11], 1920–2013^[12], of United States^[13], awarded the Petrie Prize Lecture^[14], specialised in star formation^[15] and Guillermo Haro^[5], an astronomer^[16], 1913–1988^[17], of Mexico^[18], awarded the National Prize for Arts and Sciences^[19], specialised in astronomy^[20].

Use and Application

Herbig–Haro object is part of galaxy^[7].

Why It Matters

Herbig–Haro object draws 300 Wikipedia views per month (astronomical_object_type category, ranking #96 of 289).^[2] It has Wikipedia articles in 25 language editions, a strong signal of global cultural recognition.^[21] It is known by 18 alternative names across languages and contexts.^[22]