13 Monocerotis has been used as a standard star for the A0 Ib spectral class.[10]
Extended photometry of 13 Monocerotis from 1997 to 2000 shows irregular variation of up to 0.04 magnitudes and also a slight trend to become fainter over the period.[11] All the bright A0 - A5 supergiants analysed using Hipparcos satellite data were found to be variable, but 13 Mon was the least variable.[12]
^Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/GCVS. Originally Published in: 2009yCat....102025S. 1. Bibcode:2009yCat....102025S. Vizier catalog entry
^ abHovhannessian, R. Kh.; Hovhannessian, E. R. (2001). "Gas—Dust Shells around Some Early-Type Stars with an IR Excess (of Emission)". Astrophysics (English Translation of Astrofizika). 44 (4): 454. Bibcode:2001Ap.....44..454H. doi:10.1023/A:1014244720865. S2CID118532665.
^Morgan, W. W.; Roman, Nancy G. (1950). "Revised Standards for Supergiants on the System of the Yerkes Spectral Atlas". Astrophysical Journal. 112: 362. Bibcode:1950ApJ...112..362M. doi:10.1086/145351.
^Adelman, S. J.; Albayrak, B. (1997). "On the Variability of Early A-Type Supergiants". Information Bulletin on Variable Stars. 4541: 1. Bibcode:1997IBVS.4541....1A.