V1472 Aquilae is a pulsating binary star system in the constellation Eagle . It consists of a red giant of the spectral class M2.5 III, about the other star is currently. nothing known. The main star has the 104 (± 56) times the size, and 1100 times the brightness of the sun . The stars orbit each other over a period of 196 days.
Individual evidence
↑ HMJ Boffin, M. Hillen, JP Berger, A. Jorissen, N. Blind: Roche-lobe filling factor of mass-transferring red giants: the PIONIER view . In: Astronomy & Astrophysics . tape564 , April 1, 2014, ISSN 0004-6361 , doi : 10.1051 / 0004-6361 / 201323194 ( aanda.org [accessed June 23, 2016]).
