The Cluster AgeS Experiment (CASE) - VIII. Age and distance of the Globular Cluster 47 Tuc from the analysis of two detached eclipsing binaries Academic Article uri icon


  • ABSTRACT We use photometric and spectroscopic observations of the eclipsing binary E32 in the globular cluster 47Tuc to derive the masses, radii, and luminosities of the component stars. The system has an orbital period of 40.9d, a markedly eccentric orbit with e= 0.24, and is shown to be a member of or a recent escaper from the cluster. We obtain $M_{
    m p} = 0.862pm 0.005 , mathrm{M}_odot$, $R_{
    m p} = 1.183pm 0.003 , mathrm{R}_odot$, $L_{
    m p} = 1.65pm 0.05 , mathrm{L}_odot$ for the primary and $M_{
    m s} = 0.827pm 0.005 , mathrm{M}_odot$, $R_{
    m s} = 1.004pm 0.004 , mathrm{R}_odot$, $L_{
    m s} = 1.14pm 0.04, mathrm{L}_odot$ for the secondary. Based on these data and on an earlier analysis of the binary V69 in 47 Tuc, we measure the distance to the cluster from the distance moduli of the component stars, and, independently, from a colour surface brightness calibration. We obtain 4.550.03 and 4.500.07kpc, respectively values compatible within 1$, sigma$ with recent estimates based on Gaia DR2 parallaxes. By comparing the MR diagram of the two binaries and the colourmagnitude diagram of 47 Tuc to Dartmouth model isochrones we estimate the age of the cluster to be 12.00.5Gyr, and the helium abundance of the cluster to be Y 0.25.

published proceedings


altmetric score

  • 5.08

author list (cited authors)

  • Thompson, I. B., Udalski, A., Dotter, A., Rozyczka, M., Schwarzenberg-Czerny, A., Pych, W., ... Skowron, J.

citation count

  • 23

complete list of authors

  • Thompson, IB||Udalski, A||Dotter, A||Rozyczka, M||Schwarzenberg-Czerny, A||Pych, W||Beletsky, Y||Burley, GS||Marshall, JL||McWilliam, A||Morrell, N||Osip, D||Monson, A||Persson, SE||Szymański, MK||Soszyński, I||Poleski, R||Ulaczyk, K||Wyrzykowski, Ł||Kozłowski, S||Mróz, P||Pietrukowicz, P||Skowron, J

publication date

  • January 2020