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- Effective_radius abstract "The effective radius of a galaxy is the radius at which one half of the total light of the system is emitted interior to this radius. This assumes the galaxy is spherically symmetric. This is an important length scale in de Vaucouleurs law which is given as:where is the surface brightness at . Note that at ,Thus the central surface brightness is approximately .".
- Effective_radius thumbnail Half_light_radius_simple.svg?width=300.
- Effective_radius wikiPageID "8082019".
- Effective_radius wikiPageRevisionID "559036813".
- Effective_radius hasPhotoCollection Effective_radius.
- Effective_radius subject Category:Physical_quantities.
- Effective_radius type Abstraction100002137.
- Effective_radius type Measure100033615.
- Effective_radius type PhysicalQuantities.
- Effective_radius comment "The effective radius of a galaxy is the radius at which one half of the total light of the system is emitted interior to this radius. This assumes the galaxy is spherically symmetric. This is an important length scale in de Vaucouleurs law which is given as:where is the surface brightness at . Note that at ,Thus the central surface brightness is approximately .".
- Effective_radius label "Effective radius".
- Effective_radius label "Effektiver Radius".
- Effective_radius label "Promień półświatła".
- Effective_radius label "Rayon effectif".
- Effective_radius sameAs Effektiver_Radius.
- Effective_radius sameAs Rayon_effectif.
- Effective_radius sameAs Promień_półświatła.
- Effective_radius sameAs m.026qrzl.
- Effective_radius sameAs Q1295998.
- Effective_radius sameAs Q1295998.
- Effective_radius sameAs Effective_radius.
- Effective_radius wasDerivedFrom Effective_radius?oldid=559036813.
- Effective_radius depiction Half_light_radius_simple.svg.
- Effective_radius isPrimaryTopicOf Effective_radius.