Faịlụ:HRDiagram.png
Otu nyochaa a ha:526 × 599 piksels Ndị ọzọ mkpebi:211 × 240 piksels | 421 × 480 piksels | 720 × 820 piksels.
Failụ si na nke mbu (720 × 820 pixel, ívù akwukwo orunótu: 19 KB, MIME nke: image/png)
| Nkówá | Hertzsprung–Russell diagram. A plot of luminosity (absolute magnitude) against the colour of the stars ranging from the high-temperature blue-white stars on the left side of the diagram to the low temperature red stars on the right side. "This diagram below is a plot of 22000 stars from the Hipparcos Catalogue together with 1000 low-luminosity stars (red and white dwarfs) from the Gliese Catalogue of Nearby Stars. The ordinary hydrogen-burning dwarf stars like the Sun are found in a band running from top-left to bottom-right called the Main Sequence. Giant stars form their own clump on the upper-right side of the diagram. Above them lie the much rarer bright giants and supergiants. At the lower-left is the band of white dwarfs – these are the dead cores of old stars which have no internal energy source and over billions of years slowly cool down towards the bottom-right of the diagram." Converted to png and compressed with pngcrush. |
| Mkpọlọ́gwụ̀ | The Hertzsprung Russell Diagram |
| Odé ákwụ́kwọ́ | Richard Powell |
| Ọdà (Í jí kwá usòrò nke) |
   This file is licensed under the Creative Commons Attribution-Share Alike 2.5 Generic license.
|
| Nke ya ozor |
[]
|
|
This diagram image could be re-created using vector graphics as an SVG file. This has several advantages; see Commons:Media for cleanup for more information. If an SVG form of this image is available, please upload it and afterwards replace this template with
{{vector version available|new image name}}.
It is recommended to name the SVG file “HRDiagram.svg”—then the template Vector version available (or Vva) does not need the new image name parameter. |
Ịta nke usòrò
Bìri èhì/ogè k'ị hụ òtù ụ̀fa dị̀ m̀gbè ahụ̀.
| Èhì/Ogè | Mbọ-aka | Ógólógó na asaá | Òjìème | Nkwute | |
|---|---|---|---|---|---|
| dị ùgbu â | 18:32, 18 Mee 2011 | 720 × 820 (19 KB) | Saibo | Reverted to version as of 03:42, 3 March 2007. Commons:Avoid_overwriting_existing_files | |
| 22:17, 25 Maachị 2011 | 720 × 820 (59 KB) | Tomruen | black labels | ||
| 18:25, 25 Maachị 2011 | 720 × 820 (34 KB) | Tomruen | invert colors, white background | ||
| 03:42, 3 Maachị 2007 | 720 × 820 (19 KB) | Falcorian | {{Information |Description=Hertzsprung-Russell diagram. A plot of luminosity (absolute magnitude) against the colour of the stars ranging from the high-temperature blue-white stars on the left side of the diagram to the low temperature red stars on the ri |
Ojiji faịlụ
Ihe ndị na-eso ihe eji Ihu akwụkwọ eme na faịlụ a:
Ejiji failụ zụrụ ọha
Wikis ndi a edeputara na eji kwa failụ a:
- Ihe eji na af.wikipedia.org
- Ihe eji na af.wiktionary.org
- Ihe eji na ar.wikipedia.org
- Ihe eji na bg.wikipedia.org
- Ihe eji na bn.wikipedia.org
- Ihe eji na bs.wikipedia.org
- Ihe eji na ca.wikipedia.org
- Ihe eji na cv.wikipedia.org
- Ihe eji na cy.wikipedia.org
- Ihe eji na de.wikipedia.org
- Ihe eji na de.wikibooks.org
- Ihe eji na el.wikipedia.org
- Ihe eji na en.wikipedia.org
- Main sequence
- User:TimothyPilgrim
- Subgiant
- Red clump
- Hertzsprung gap
- Wikipedia:Today's featured article/March 31, 2009
- Wikipedia:Today's featured article/March 2009
- Hertzsprung–Russell diagram
- Portal:Astronomy/Featured/October 2009
- HD 114613
- HD 154088
- HD 108063
- HD 41742 and HD 41700
- User:Kazkaskazkasako/Books/Physical sciences
- User:Redwoodking
- Robust Regression and Outlier Detection
- Arne Slettebak
- Ihe eji na en.wikibooks.org
- Ihe eji na eo.wikipedia.org
- Ihe eji na es.wikipedia.org
- Ihe eji na et.wikipedia.org
- Ihe eji na fa.wikipedia.org
- Ihe eji na fa.wikibooks.org
- Ihe eji na fr.wikipedia.org
Lee more global usage of this file.