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Hubble's constant determined using very-long baseline interferometry of a supernova

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Abstract

Determination of the angular expansion velocity of the radiosphere of the supernova SN1979c in the galaxy Ml00 in the Virgo cluster, combined with determination of the radial expansion velocity of the photosphere, yields an estimate of the distance to the Virgo cluster centre of Dvirgo = 19+8−6 Mpc and of the Hubble constant of H0=65+35−25 km s−1 Mpc−1, where the uncertainties given are based on conservative, but reasonable estimates of all significant errors and are intended to represent 90% confidence intervals.

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Author information

Author notes

  1. J. M. Marcaide

    Present address: Siemens AG, Postfach, 700074, München, FRG

  2. K. W. Weiler

    Present address: E. O. Hurlburt Centre for Space Research, Naval Research Laboratory, Washington, DC, 20375-5000, USA

Authors and Affiliations

  1. Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts, 02138, USA

    N. Bartel, I. I. Shapiro, M. V. Gorenstein & C. R. Gwinn

  2. NEROC Haystack Observatory, Westford, Massachusetts, 01886, USA

    A. E. E. Rogers

  3. Max-Planck-Institut für Radioastronomie, Bonn, FRG

    J. M. Marcaide

  4. National Science Foundation, Washington, DC, 20550, USA

    K. W. Weiler

Authors
  1. N. Bartel
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  2. A. E. E. Rogers
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  3. I. I. Shapiro
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  4. M. V. Gorenstein
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  5. C. R. Gwinn
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  6. J. M. Marcaide
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  7. K. W. Weiler
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Bartel, N., Rogers, A., Shapiro, I. et al. Hubble's constant determined using very-long baseline interferometry of a supernova. Nature 318, 25–30 (1985). https://doi.org/10.1038/318025a0

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