van Leeuwen, F. (November 2007), «Validation of the new Hipparcos reduction», Astronomy and Astrophysics474 (2): 653–664, doi:10.1051/0004-6361:20078357
Walczak, P.; Daszyńska-Daszkiewicz, J. (December 2010), «Complex asteroseismology of the hybrid B-type pulsator γ Pegasi: A test of stellar opacities», Astronomische Nachrichten331 (9/10): 1057–1060, doi:10.1002/asna.201011456
McNamara, D. H. (June 1953), «Gamma Pegasi: A Beta Canis Majoris Star of Small Velocity Amplitude», Publications of the Astronomical Society of the Pacific65 (384): 144, doi:10.1086/126561
Fitzpatrick, E. L.; Massa, D. (March 2005), «Determining the Physical Properties of the B Stars. II. Calibration of Synthetic Photometry», The Astronomical Journal129 (3): 1642–1662, doi:10.1086/427855
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, doi:10.1002/asna.200911355
Huang, W.; Wallerstein, G.; Stone, M. (2012), «A catalogue of Paschen-line profiles in standard stars», Astronomy & Astrophysics547: A62, doi:10.1051/0004-6361/201219804
Abt, Helmut A.; Levato, Hugo; Grosso, Monica (July 2002), «Rotational Velocities of B Stars», The Astrophysical Journal573 (1): 359–365, doi:10.1086/340590. The zero value is for v sin i, so v and/or i must be small.