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Extreme Galactic-Winds and Starburst in IR Mergers and IR QSOs

S. Lipari·D. Sanders·R. Terlevich·S. Veilleux·R. Diaz·Y. Taniguchi·W. Zheng·D. Kim·Z. Tsvetanov·G. Carranza·H. Dottori
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Abstract

We report -as a part of a long-term study of mergers and IR QSOs- detailed spectroscopic evidences for outflow (OF) and/or Wolf Rayet features in: (i) low velocity OF in the ongoing mergers NGC 4038/39 and IRAS 23128-5919; (ii) extreme velocity OF (EVOF) in the QSOs IRAS 01003-2238 and IRAS 13218+0552; (iii) OF and EVOF in a complete sample of ultra-luminous IR galaxies/QSOs ("The IRAS 1 Jy MKO-KPNO Survey", of 118 objects). We found EVOF in IRAS 11119+3257, 14394+5332, 15130+1958 and 15462-0450. The OF components detected in these objects were mainly associated to starburst processes: i.e., to galactic-winds generated in multiple type II SN explosions and massive stars. The EVOF were detected in objects with strong starburst plus obscured IR QSOs; which suggest that interaction of both processes could generate EVOF. In addition, we analyze the presence of Wolf Rayet features in the large sample of Bright PG-QSOs (Boroson and Green 1992), and nearby mergers and galactic-wind galaxies. We found clear WR features in the Fe II QSOs (type I): PG 1244+026, 1444+407, 1448+273, 1535+547; and in the IR merger Arp 220. HST archive images of IR+BAL QSOs show in practically all of these objects "arc or shell" features probably associated to galactic-winds (i.e., to multiple type II SN explosions) and/or merger processes. Finally, we discuss the presence of extreme starburst and galactic wind as a possible evolutive link between IR merger and IR QSOs; where the relation between mergers and extreme starburst (with powerful galactic-winds) plays in important role, in the evolution of galaxies.

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S. Lipari, D. Sanders, R. Terlevich, S. Veilleux, R. Diaz, Y. Taniguchi, W. Zheng, D. Kim, Z. Tsvetanov, G. Carranza, H. Dottori. 2000-07-20. Extreme Galactic-Winds and Starburst in IR Mergers and IR QSOs. https://doi.org/10.1046/j.1365-8711.2003.06309.x

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