59m Photometric period in the dwarf nova V 485 Centauri

被引：0
|
作者：
机构：
来源：
| 1600年 / 267期
关键词：
D O I：
暂无
中图分类号：
学科分类号：
摘要：
引用
收藏
相关论文
共 45 条
  • [41] The shortest period M dwarf eclipsing system BW3V38 -: II.: Determination of absolute elements
    Maceroni, C
    Montalbán, J
    ASTRONOMY & ASTROPHYSICS, 2004, 426 (02) : 577 - 585
  • [42] The shortest period M dwarf eclipsing system BW3 V38 II. Determination of absolute elements
    Maceroni, C.
    Montalbán, J.
    Astronomy and Astrophysics, 1600, 426 (02): : 577 - 585
  • [43] Extensive photometry of the WZ Sge-type dwarf nova V455 And (HS2331+3905): Detection of negative superhumps and coherence features of the short-period oscillations
    Kozhevnikov, V. P.
    NEW ASTRONOMY, 2015, 41 : 59 - 66
  • [44] Cataclysmic and close binaries in star clusters. V. Erupting dwarf novae, faint blue stars, X-ray sources, and the classical nova in the core of M80
    Shara, MM
    Hinkley, S
    Zurek, DR
    ASTROPHYSICAL JOURNAL, 2005, 634 (02): : 1272 - 1285
  • [45] Investigating magnetic activity in very stable stellar magnetic fields Long-term photometric and spectroscopic study of the fully convective M4 dwarf V374 Pegasi
    Vida, K.
    Kriskovics, L.
    Olah, K.
    Leitzinger, M.
    Odert, P.
    Kovari, Zs.
    Korhonen, H.
    Greimel, R.
    Robb, R.
    Csak, B.
    Kovacs, J.
    ASTRONOMY & ASTROPHYSICS, 2016, 590
12345