A Shock-Induced Pair of Superbubbles in the High-Redshift Powerful Radio Galaxy MRC 0406-244

We present new optical spectroscopy of the high-redshift powerful radio galaxy MRC 0406\(-\)244 at redshift of 2.429. We find that the two extensions toward NW and SE probed in the rest-frame ultraviolet image are heated mainly by the nonthermal continuum of the active galactic nucleus. However, eac...

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Veröffentlicht in:	arXiv.org 2001-08
Hauptverfasser:	Taniguchi, Yoshiaki, Ohyama, Youichi, Murayama, Takashi, Yoshida, Michitoshi, Kashikawa, Nobunari, Iye, Masanori, Aoki, Kentaro, Sasaki, Toshiyuki, Kosugi, George, Takata, Tadafumi, Saito, Yoshihiko, Kawabata, Koji S, Sekiguchi, Kazuhiro, Okita, Kiichi, Shimizu, Yasuhiro, Inata, Motoko, Ebizuka, Noboru, Ozawa, Tomohiko, Yadomaru, Yasushi, Taguchi, Hiroko, Shioya, Yasuhiro, Nishiura, Shingo, Sudou, Hiroshi, Nagao, Tohru, Noda, Saeko, Kakazu, Yuko, Ajiki, Masaru, Fujita, Shinobu S, Kobayashi, Rie R
Format:	Artikel
Sprache:	eng
Schlagworte:	Active galactic nuclei Galaxies Morphology Radio galaxies Radio jets (astronomy) Red shift
Online-Zugang:	Volltext
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