Tugna:HRDiagram.png

Tiddi n azaraskan agi : 526 × 599 iferdisen n tugna. Tibuda nniḍen : 211 × 240 iferdisen n tugna | 421 × 480 iferdisen n tugna | 720 × 820 iferdisen n tugna.

Afaylu aneṣli ‎(720 × 820 pixel, tiddi n ufaylu: 19 KB/KO, anaw n MIME: image/png)

Afaylu agi yusad seg : Wikimedia Commons. Ahat yeseqdec deg isenfaṛen nniḍen. Aglam-is ɣef asebter n aglam ye beqqeḍ ddaw-agi.

AglamHRDiagram.png	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.
Aɣbalu	The Hertzsprung Russell Diagram
Ameskar	Richard Powell
Tasiregt (Tulsa n useqdec n ufaylu-agi)	Ce fichier est disponible selon les termes de la licence Creative Commons Attribution – Partage dans les Mêmes Conditions 2.5 Générique Ɣuṛ-k tilelli: i beṭṭu – akken ad tneɣleḍ, ad tzuzreḍ neɣ ad tebḍuḍ amahil-agi i uṣeggem – i uṣeggem n umahil Ddaw n tiwtilin-agi: bab – Yessefk ad d-bedreḍ isem n umeskar aneṣli s wudem yettwammlen sɣuṛ ameskar n umahil neɣ bab n izerfan i k-imudden tasiregt (mačči s wudem yemmalen am akken yettmuddu-yak afus neɣ yeqbel aseqdec-it n umahil). bḍut akken yella – Ma tbeddleḍ, teskelteḍ, neɣ tebniḍ ɣef umahil-agi, yessefk ad tezzuzreḍ amahil i d-yeffɣen ɣas ddaw n turagt-nni neɣ turagt icuban ɣuṛ-s. CC BY-SA 2.5 truetrue (See Copyright)
Autres versions	[beddel] Hertzsprung–Russell diagram Afrikaans Afrikaans (alt) català čeština English English (alt) español français galego italiano magyar oʻzbekcha polski slovenčina suomi (alt) svenska беларуская қазақша русский հայերեն 日本語中文（繁體） עברית עברית العربية Sun + Sirius sparse català Deutsch (PNG) Deutsch English (PNG) English español galego Lëtzebuergesch Türkçe Well-known stars in the Milky Way Afrikaans English English (alt) Kiswahili Deutsch български

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Amazray n ufaylu

Senned ɣef yiwen azmez d usrag iwakken ad ẓṛeḍ afaylu aken yella deg imir nni.

	Azemz/Ssaɛa	Iseggiwen	Amseqdac	Awennit
Lux a	18 Mayyu 2011 à 18:32	720 × 820 (19 KB/KO)	Saibo	Reverted to version as of 03:42, 3 March 2007. Commons:Avoid_overwriting_existing_files
	25 Meɣres 2011 à 22:17	720 × 820 (59 KB/KO)	Tomruen	black labels
	25 Meɣres 2011 à 18:25	720 × 820 (34 KB/KO)	Tomruen	invert colors, white background
	3 Meɣres 2007 à 03:42	720 × 820 (19 KB/KO)	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