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Elliptical Galaxies and Non-Uniformities in the Hubble Flow

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Galaxy Distances and Deviations from Universal Expansion

Part of the book series: NATO ASI Series ((ASIC,volume 180))

Abstract

We have obtained spectroscopic and photometric data for 400 elliptical galaxies that permit us to predict distances to individual galaxies with accuracies of ±23%. Systematic velocities relative to a smooth Hubble flow are observed that are most straightforwardly interpreted as a bulk motion of approximately 700 km/s towards l=299°, b=+1° for galaxies within 60 h-1 Mpc of the Local Group, A preliminary estimate for the rms motion of elliptical galaxy gruops relative to the bulk motion is 300 km/s. Spiral galaxies studied by Aaronson et al. and by Rubin et al. yield similar results for both the bulk and the rms motion.

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References

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© 1986 D. Reidel Publishing Company

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Burstein, D. et al. (1986). Elliptical Galaxies and Non-Uniformities in the Hubble Flow. In: Madore, B.F., Tully, R.B. (eds) Galaxy Distances and Deviations from Universal Expansion. NATO ASI Series, vol 180. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-4702-3_22

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  • DOI: https://doi.org/10.1007/978-94-009-4702-3_22

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-8591-5

  • Online ISBN: 978-94-009-4702-3

  • eBook Packages: Springer Book Archive

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