鳳凰座SX型變星

鳳凰座SX型變星變星的一種,這些恆星的亮度表現出週期在0.03~0.08天 (0.7~1.9小時) 的脈動變化,它們的光譜類型在A2~F5,星等變化可以達到0.7等[1]。相較於太陽,這些恆星的金屬量較低,這意味著其它元素相較於的豐度是較低的。在相同分類的恆星中,它們也有著較高的空間速度和低光度[2][3],這些屬性使鳳凰座SX型變星和表兄弟的盾牌座δ型變星有所區別。後著有著較成的週期、高金屬量和較大的變光幅度[4]

鳳凰座SX型變星主要分出現在球狀星團銀暈中,變光週期和亮度明顯的有週光關係[5]。已知所有有鳳凰座SX型變星的球狀星團內都有藍掉隊星[6],這些恆星看起來比在同一個星團中有著相同亮度的主序星更藍 (有著更高的溫度)[7]

參考資料

  1. . General Catalogue of Variable Stars. Moscow, Russia: Russian Foundation for Basic Research, Sternberg Astronomical Institute. [2010-03-17].
  2. Burki, G.; Mayor, M. . . Christchurch, New Zealand: Dordrecht, D. Reidel Publishing Co.: 392. 1986. Bibcode:1986IAUS..118..385B.
  3. Breger, M. . Astrophysical Journal, Part 1. Jan 1980, 235: 156. Bibcode:1980ApJ...235..153B. doi:10.1086/157620.
  4. McNamara, D. H. . Astronomical Journal. 1995, 109 (4): 1751–1756. Bibcode:1995AJ....109.1751M. doi:10.1086/117405. 已忽略未知参数|month=(建议使用|date=) (帮助)
  5. Templeton, Matthew. . American Association of Variable Star Observers. (原始内容存档于2006-10-26).
  6. Jeon, Young-Beom; Lee, Myung Gyoon; Kim, Seung-Lee; Lee, Ho. . The Astronomical Journal. July 2004, 128 (1): 11. Bibcode:2004AJ....128..287J. arXiv:astro-ph/0404069. doi:10.1086/421735.
  7. Santolamazza, P.; Marconi, M.; Bono, G.; Caputo, F.; Cassisi, S.; Gilliland, R. L. . The Astrophysical Journal. June 2001, 554 (2): 1124–1140. Bibcode:2001ApJ...554.1124S. arXiv:astro-ph/0102029. doi:10.1086/321408.
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