ﻻ يوجد ملخص باللغة العربية
Observations from the first flight of the Medium Scale Anisotropy Measurement (MSAM1-92) are analyzed to search for the Sunyaev-Zeldovich (SZ) effect towards the Coma cluster. This balloon-borne instrument uses a $28arcmin$ FWHM beam and a three position chopping pattern with a throw of $pm40arcmin$. With spectral channels at 5.7, 9.3, 16.5, and 22.6~icm, the observations simultaneously sample the frequency range where the SZ spectral distortion in the intensity transitions from a decrement to an increment and where the fractional intensity change is substantially larger than in the Rayleigh-Jeans region. We set limits on the Comptonization parameter integrated over our antenna pattern, $Delta y leq 8.0 times 10^{-5}$($2 sigma$). For a spherically symmetric isothermal model, this implies a central Comptonization parameter, $y_o leq 2.0 times 10^{-4}$, or a central electron density, $n_o leq 5.8 times10^{-3}$cm$^{-3}h_{50}$, a result consistent with central densities implied by X-ray brightness measurements and central Comptonization estimates from lower frequency observations of the SZ effect.
The Sunyaev-Zeldovich (SZ) effect was previously measured in the Coma cluster by the Owens Valley Radio Observatory and Millimeter and IR Testa Grigia Observatory experiments and recently also with the Wilkinson Microwave Anisotropy Probe satellite.
Studying galaxy clusters through their Sunyaev-Zeldovich (SZ) imprint on the Cosmic Microwave Background has many important advantages. The total SZ signal is an accurate and precise tracer of the total pressure in the intra-cluster medium and of clu
X-ray observations of an entropy floor in nearby groups and clusters of galaxies offer evidence that important non-gravitational processes, such as radiative cooling and/or preheating, have strongly influenced the evolution of the intracluster medium
The Planck collaboration has recently published precise and resolved measurements of the Sunyaev-Zeldovich effect in Abell 1656 (the Coma cluster of galaxies), so directly gauging the electron pressure profile in the intracluster plasma. On the other
In this paper we probe the hot, post-shock gas component of quasar-driven winds through the thermal Sunyaev-Zeldovich (tSZ) effect. Combining datasets from the Atacama Cosmology Telescope, the $textit{Herschel}$ Space Observatory, and the Very Large