English

Feedback and feeding in the context of galaxy evolution with SPICA: direct characterization of molecular outflows and inflows

Astrophysics of Galaxies 2018-03-22 v1

Abstract

A far-infrared observatory such as the {\it SPace Infrared telescope for Cosmology and Astrophysics} ({\it SPICA}), with its unprecedented spectroscopic sensitivity, would unveil the role of feedback in galaxy evolution during the last 10\sim10 Gyr of the Universe (z=1.52z=1.5-2), through the use of far- and mid-infrared molecular and ionic fine structure lines that trace outflowing and infalling gas. Outflowing gas is identified in the far-infrared through P-Cygni line shapes and absorption blueshifted wings in molecular lines with high dipolar moments, and through emission line wings of fine-structure lines of ionized gas. We quantify the detectability of galaxy-scale massive molecular and ionized outflows as a function of redshift in AGN-dominated, starburst-dominated, and main-sequence galaxies, explore the detectability of metal-rich inflows in the local Universe, and describe the most significant synergies with other current and future observatories that will measure feedback in galaxies via complementary tracers at other wavelengths.

Keywords

Cite

@article{arxiv.1710.02356,
  title  = {Feedback and feeding in the context of galaxy evolution with SPICA: direct characterization of molecular outflows and inflows},
  author = {E. González-Alfonso and L. Armus and F. J. Carrera and V. Charmandaris and A. Efstathiou and E. Egami and J. A. Fernández-Ontiveros and J. Fischer and G. L. Granato and C. Gruppioni and E. Hatziminaoglou and M. Imanishi and N. Isobe and H. Kaneda and D. Koziel-Wierzbowska and M. A. Malkan and J. Martin-Pintado and S. Mateos and H. Matsuhara and G. Miniutti and T. Nakagawa and F. Pozzi and F. Rico-Villas and G. Rodighiero and P. Roelfsema and L. Spinoglio and H. W. W. Spoon and E. Sturm and F. van der Tak and C. Vignali and L. Wang},
  journal= {arXiv preprint arXiv:1710.02356},
  year   = {2018}
}

Comments

This paper belongs to the SPICA Special Issue on PASA. Accepted for publication in PASA