Английская Википедия:Camelopardalis OB1

Материал из Онлайн справочника
Перейти к навигацииПерейти к поиску

Шаблон:Infobox stellar association

Camelopardalis OB1 (Cam OB1) is a group of young stars that share a common origin and a similar motion through space, but, as a whole, are no longer gravitationally bound. The name indicates this stellar association is located in the area of the Camelopardalis constellation which includes a number of massive, short-lived OB stars. The association is ~Шаблон:Cvt distant from the Sun, with members lying between Шаблон:Val and Шаблон:Val away. It is located on the edge of the local Orion Arm of the Milky Way galaxy and lies outside the traditional Gould Belt.[1]

The member stars were first classified as an association by Georg (Jiří) Alter, B. Y. Israel, and Jaroslav Ruprecht in 1966.[2][3] The open cluster NGC 1502 is considered a member of Cam OB1.[1] A second cluster in Cam OB1, G144.9+0.4, was identified in 2010 with 91 OB candidate stars.[4] Excluding these clusters, two O-type and 35 B-type stars have been identified as members.[1] Stars have been forming in the region of this association for the last 100 million years,[3] and star formation is still in progress.[1] It has a combined mass of ~5,000 times the mass of the Sun.[5]

References

Шаблон:Reflist

  1. 1,0 1,1 1,2 1,3 Ошибка цитирования Неверный тег <ref>; для сносок Straižys_Laugalys_2007 не указан текст
  2. Ошибка цитирования Неверный тег <ref>; для сносок alter1966 не указан текст
  3. 3,0 3,1 Ошибка цитирования Неверный тег <ref>; для сносок Lyder2001 не указан текст
  4. Ошибка цитирования Неверный тег <ref>; для сносок Lin_et_al_2013 не указан текст
  5. Ошибка цитирования Неверный тег <ref>; для сносок Melnik_Dambis_2020 не указан текст