The distance to M51

Kristen B W McQuinn, Evan D. Skillman, Andrew E. Dolphin, Danielle Berg, Robert Kennicutt

    Research output: Contribution to journalArticlepeer-review

    40 Scopus citations

    Abstract

    Great investments of observing time have been dedicated to the study of nearby spiral galaxies with diverse goals ranging from understanding the star formation process to characterizing their dark matter distributions. Accurate distances are fundamental to interpreting observations of these galaxies, yet many of the best studied nearby galaxies have distances based on methods with relatively large uncertainties. We have started a program to derive accurate distances to these galaxies. Here we measure the distance to M51 - the Whirlpool galaxy - from newly obtained Hubble Space Telescope optical imaging using the tip of the red giant branch method. We measure the distance modulus to be 8.58 ± 0.10 Mpc (statistical), corresponding to a distance modulus of 29.67 ± 0.02 mag. Our distance is an improvement over previous results as we use a well-calibrated, stable distance indicator, precision photometry in a optimally selected field of view, and a Bayesian Maximum Likelihood technique that reduces measurement uncertainties.

    Original languageEnglish (US)
    Article number21
    JournalAstrophysical Journal
    Volume826
    Issue number1
    DOIs
    StatePublished - Jul 20 2016

    Keywords

    • Hertzsprung-Russell and C-M diagrams
    • galaxies: distances and redshifts
    • galaxies: spiral

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