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20 April 2024
 
  » arxiv » astro-ph/0109425

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Infrared Mass-to-Light Profile Throughout the Infall Region of the Coma Cluster
K. Rines ; M.J. Geller ; M.J. Kurtz ; A. Diaferio ; T.H. Jarrett ; J.P. Huchra ;
Date 24 Sep 2001
Journal Astrophys.J. 561 (2001) L41
Subject astro-ph
AbstractUsing a redshift survey of 1779 galaxies and photometry from the 2-Micron All-Sky Survey (2MASS) covering 200 square degrees, we calculate independent mass and light profiles for the infall region of the Coma cluster of galaxies. The redshift survey is complete to $K_s=12.2$ (622 galaxies), 1.2 magnitudes fainter than $M^*_{K_s}$ at the distance of Coma. We confirm the mass profile obtained by Geller, Diaferio, & Kurtz. The enclosed mass-to-light ratio measured in the $K_s$ band is approximately constant to a radius of $10 Mpc$, where $M/L_{K_s}= 75pm 23mlsun$, in agreement with weak lensing results on similar scales. Within $2.5Mpc$, X-ray estimates yield similar mass-to-light ratios (67$pm32h$). The constant enclosed mass-to-light ratio with radius suggests that K-band light from bright galaxies in clusters traces the total mass on scales $lesssim10 Mpc$. Uncertainties in the mass profile imply that the mass-to-light ratio inside $r_{200}$ may be as much as a factor of 2.5 larger than that outside $r_{200}$. These data demonstrate that K-band light is not positively biased with respect to the mass; we cannot rule out antibias. These results imply $Omega_m = 0.17 pm 0.05$. Estimates of possible variations in $M/L_{K_s}$ with radius suggest that the density parameter is no smaller than $Omega_m approx 0.08$.
Source arXiv, astro-ph/0109425
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