また、古代アラビアでは、この星とわし座δ星、わし座θ星で、アル・ミザン(ألميزان、秤の棒)を構成する[16]。Technical Memorandum 33-507 - A Reduced Star Catalog Containing 537 Named Starsという星表によると、わし座δ星はアル・ミザンI、わし座η星はアル・ミザンII、わし座θ星はアル・ミザンIIIと呼ばれる[17]。
^Nordgren, Tyler E. et al. (December 1999), “Stellar Angular Diameters of Late-Type Giants and Supergiants Measured with the Navy Prototype Optical Interferometer”, The Astronomical Journal118 (6): 3032-3038, Bibcode: 1999AJ....118.3032N, doi:10.1086/301114.
^ abcdTetzlaff, N.; Neuhäuser, R.; Hohle, M. M. (January 2011), “A catalogue of young runaway Hipparcos stars within 3 kpc from the Sun”, Monthly Notices of the Royal Astronomical Society410 (1): 190-200, Bibcode: 2011MNRAS.410..190T, doi:10.1111/j.1365-2966.2010.17434.x.
^ abcLuck, R. E.; Lambert, D. L. (May 1981), “The abundances of carbon, nitrogen, and oxygen in the atmospheres of Cepheid variables - Evidence for helium enrichment”, Astrophysical Journal, Part 1245: 1018-1034, Bibcode: 1981ApJ...245.1018L, doi:10.1086/158879.
^Hohle, M. M.; Neuhäuser, R.; Schutz, B. F. (April 2010), “Masses and luminosities of O- and B-type stars and red supergiants”, Astronomische Nachrichten331 (4): 349, Bibcode: 2010AN....331..349H, doi:10.1002/asna.200911355.
^Wiktorowicz, Sloane J.; Matthews, Keith (December 2008), “A High-Precision Optical Polarimeter to Measure Inclinations of High-Mass X-Ray Binaries”, The Publications of the Astronomical Society of the Pacific120 (874): 1282-1297, Bibcode: 2008PASP..120.1282W, doi:10.1086/595966.
^Gray, David F.; Stevenson, Kevin B. (April 2007), “Spectroscopic Determination of Radius Changes of Cepheid Variable Stars”, The Publications of the Astronomical Society of the Pacific119 (854): 398-406, Bibcode: 2007PASP..119..398G, doi:10.1086/518128