TY Coronae Australis (abbreviated as TY CrA), is a young star system around 3 million years old in the constellationCorona Australis. It is composed of a blue-white B-class star around triple the Sun's mass and a cooler smaller companion around half its mass (or 1.6 times that of the Sun). The system is an eclipsing binary with a period of 2.8 days.
↑Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues. 2237. Bibcode:2002yCat.2237....0D.
↑Vieira, S. L. A.; Corradi, W. J. B.; Alencar, S. H. P.; Mendes, L. T. S.; Torres, C. A. O.; Quast, G. R.; Guimarães, M. M.; Da Silva, L. (2003). "Investigation of 131 Herbig Ae/Be Candidate Stars". The Astronomical Journal. 126 (6): 2971. Bibcode:2003AJ....126.2971V. doi:10.1086/379553.
↑Innes, R. T. A. (November 1916). "The Variable Stars and Nebulae Near R Corona Australe". Circular of the Union Observatory Johannesburg. 36: 282–284. Bibcode:1916CiUO...36..282I.