High Energy Astronomy Observatory 1

Nelson Owen）探測到了該聯星的電波發射。1978年使用HEAO1（英语：High Energy Astronomy Observatory 1）衛星證明它是軟X射線源。 這個雙線光譜聯星系統由一顆演化中的K型次巨星和一顆普通的G型主序星組成。這兩顆恆星

Astronomical Observatory Circular, 1984, 8: 59−67, Bibcode:1984SAAOC...8...59C.  Chini, R.; et al, spectroscopic survey on the multiplicity of high-mass stars

001 （英语）.  IceCube Neutrino Observatory. [2015-01-13]. （原始内容存档于2015-01-12）.  IceCube Collaboration*. Evidence for High-Energy Extraterrestrial Neutrinos

Lyubchik, Yu.; Tennyson, J.; Pinfield, D. J. Spectral energy distribution for GJ406. Astronomy and Astrophysics. 2006, 447 (2): 709–717 [2007-07-18].

Mysterious Microquasar （页面存档备份，存于互联网档案馆）, press release, National Radio Astronomy Observatory, October 26, 2004, accessed on line September 14, 2007. Murata,