We present results of an imaging observation of the central region of a giant radio galaxy B1358+305. The classical, standard scenario of Fanaroff-Riley II radio galaxies suggests that shock-produced hot electrons contained in a radio galaxy are a good reservoir of the jet-supplied energy from active nuclei. The aim of our observation is to search for the Sunyaev-Zel'dovich effect (SZE) induced by these hot electrons. The observation was performed at 21?GHz with the Nobeyama 45 m telescope. Deep imaging observation of a wide region of size 67 × 67 with the beam size θHPBW = 812 enables the most detailed examination of the possible thermal energy of electrons contained in a radio galaxy. The resultant intensity fluctuation is 0.56?mJy?beam–1 (in terms of the Compton y-parameter, y = 1.04 × 10–4) at a 95% confidence level. The intensity fluctuation obtained with imaging analysis sets the most stringent upper limit on the fluctuations in the central region of a giant radio galaxy obtained so far, and our results will be a toehold for future plans of SZE observation in a radio galaxy.
展开▼
