Issue |
A&A
Volume 527, March 2011
|
|
---|---|---|
Article Number | L10 | |
Number of page(s) | 6 | |
Section | Letters | |
DOI | https://doi.org/10.1051/0004-6361/201016169 | |
Published online | 08 February 2011 |
Online material
Spectroscopic cluster members of XMMU J1007.4+1237.
Properties of the galaxy cluster XMMU J1007.4+1237.
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Fig. 2
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. |
Open with DEXTER |
© ESO, 2011
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