Mmeslay:Agezlan awraɣ
Agezlan awraɣ neɣ Itran n welkam agejdan anaw-G d itri seg welkam agejdan yeṭṭafaren talmest taylalant G yakk d tseddart n usfijjej V. Takura tamudemant n yitran am wid-ak-a tga gar n 0,8 alamma d 1,2 n tkurawin tinafukin akken i lan (sɛan) taẓɣelt tajummant yattawaṭen seg 5,300 alamma d 6000 C°.[1] dɣa itran n telmest G atnan di tallit n usuɣel n u hidrujin ɣer Ahilium deg weɣyay-is s temhalt n wezday aɣisan i d-ittilin deh yitran n welkam agejdan yakk.[2] Tafukt tga d amedya igerrzen yerna d win i d-yufraren yakk deg tegrawt n yitran n G. Yal yiwet n tsint yettili-d wezday n wazal n 600 n imelyan n iṭunnen seg uhidṛuj ɣer uhilium, ayen yettarran azal n 4 n imelyan n iṭunnen seg tenga ɣer tfasa.[3]
- ↑ Empirical bolometric corrections for the main-sequence, G. M. H. J. Habets and J. R. W. Heintze, Astronomy and Astrophysics Supplement 46 (November 1981), pp. 193–237. Archived 2017-11-09 at the Wayback Machine
- ↑ Stellar Evolution: Main Sequence to Giant, class notes, Astronomy 101, Valparaiso University, accessed on line June 19, 2007. [dead link] Archived 2020-05-13 at the Wayback Machine
- ↑ Why Does The Sun Shine?, lecture, Barbara Ryden, Astronomy 162, Taseddawit n uwanek n Ohio, accessed on line June 19, 2007. Archived 2017-08-06 at the Wayback Machine
Démarrer une discussion sur Agezlan awraɣ
Les pages de discussion sont l’endroit où diverses personnes peuvent discuter de la manière d’améliorer le contenu de Wikipedia. Vous pouvez utiliser cette page pour démarrer une discussion avec les autres utilisateurs sur la façon d’améliorer la page « Agezlan awraɣ ».
