Talk:Zeta Herculis Moving Group
 | This article is rated Start-class on Wikipedia's content assessment scale. It is of interest to the following WikiProjects: | |||||||||||||
| ||||||||||||||
.jpg){kind=small}
δ Trianguli?
[edit]Some of the component star articles say that Delta Tri is a member... 76.66.197.2 (talk) 15:03, 25 November 2009 (UTC)
- I didn't have any luck finding a source to confirm that.—RJH (talk) 22:06, 27 November 2009 (UTC)
Average age?
[edit]Disagreement:
- Source: Common age [ log (age in years) = 9,8 ]. [1] So, age is 109.8 ≈ 6.3 × 109 years.
- In this article: The average age was estimated as 8.2 × 109 years.
- ^ Porto de Mello, G. F.; da Silva, L. (November 1991). "On the physical existence of the Zeta HER moving group - A detailed analysis of Phi exp 2 Pavonis". Astronomical Journal. 102: 1816–1825. Bibcode:1991AJ....102.1816P. doi:10.1086/116006.
{{cite journal}}: CS1 maint: multiple names: authors list (link)