Volume 527, March 2011
|Number of page(s)||6|
|Published online||08 February 2011|
Spectroscopic cluster members of XMMU J1007.4+1237.
Properties of the galaxy cluster XMMU J1007.4+1237.
H-band view of the 3.8′ × 3.3′ cluster environment. Red contours indicate the log-spaced projected densities of very red galaxies with colors 3 ≤ z − H ≤ 4 (see Fig. 3) spanning the levels 2–16 arcmin-2, Chandra X-ray surface brightness contours (0.7–2 keV, log-spaced) are shown in blue in the range 0.014–0.082 counts arcsec-2. 30″ (dashed) and 60″ (solid) radii around the X-ray center are marked by circles.
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© ESO, 2011
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