THE DISTANCE TO M51

• Published in: The Astrophysical journal Vol. 826; no. 1; p. 21
• Main Authors: McQuinn, Kristen. B. W., Skillman, Evan D., Dolphin, Andrew E., Berg, Danielle, Kennicutt, Robert
• Format: Journal Article
• Language: English
• Published: United States 20.07.2016
• Subjects: ACCURACY; ASTROPHYSICS, COSMOLOGY AND ASTRONOMY; Bayesian analysis; Dark matter; DISTANCE; DISTRIBUTION; GALAXIES; Hubble Space Telescope; MAXIMUM-LIKELIHOOD FIT; NONLUMINOUS MATTER; Optimization; PHOTOMETRY; RED SHIFT; SPACE; Star formation; STARS; TELESCOPES; Uncertainty
• ISSN: 0004-637X; 1538-4357
• DOI: 10.3847/0004-637X/826/1/21

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.