| Display title | Astronomy:Hubble–Reynolds law |
| Default sort key | Hubble-Reynolds law |
| Page length (in bytes) | 1,706 |
| Namespace ID | 3024 |
| Namespace | Astronomy |
| Page ID | 375509 |
| Page content language | en - English |
| Page content model | wikitext |
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| Page creator | imported>BotanyGa |
| Date of page creation | 07:59, 6 February 2024 |
| Latest editor | imported>BotanyGa |
| Date of latest edit | 07:59, 6 February 2024 |
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Description | Content |
Article description: (description)
This attribute controls the content of the description and og:description elements. | The Hubble–Reynolds law models the surface brightness of elliptical galaxies as
$ I(R)={\frac {I_{0}}{(1+R/R_{H})^{2}}} $
Where $ I(R) $ is the surface brightness at radius $ R $, $ I_{0} $ is the central brightness, and $ R_{H} $ is the radius at which the surface brightness is diminished by a factor... |
