We present the results of spectroscopic observations of galaxies associated with the diffuse X-ray emitting structure discovered by Zappacosta et al. (2002, A&A, 394, 7). After measuring the redshifts of 161 galaxies, we confirm an overdensity of galaxies with projected dimensions of at least 2 Mpc, determine its spectroscopic redshift in z = 0.401 ± 0.002, and show that it is spatially coincident with the diffuse X-ray emission. This confirms the original claim that this X-ray emission has an extragalactic nature and is due to the warm-hot intergalactic medium (WHIM). We used this value of the redshift to compute the temperature of the emitting gas. The resulting value depends on the metallicity that is assumed for the IGM, and is constrained to be between 0.3 and 0.6 keV for metallicities between 0.05 and 0.3 solar, in good agreement with the expectations from the WHIM. © ESO 2007.
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|Titolo:||A galaxy overdensity at z = 0.401 associated with an X-ray emitting structure of warm-hot intergalactic medium|
|Citazione:||Mannucci, F., Bonnoli, G., Zappacosta, L., Maiolino, R., & Pedani, M. (2007). A galaxy overdensity at z = 0.401 associated with an X-ray emitting structure of warm-hot intergalactic medium. ASTRONOMY & ASTROPHYSICS, 468(3), 807-814.|
|Appare nelle tipologie:||1.1 Articolo in rivista|
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