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Warm H_2 as a probe of massive accretion and feedback through shocks and turbulence across cosmic time

Appleton, Philip N. and Armus, Lee and Boulanger, Francois and Bradford, Charles M. and Braine, Jonathan and Bromm, Volker and Capak, Peter and Cluver, Michelle and Cooray, Asantha and Díaz-Santos, Tanio and Egami, Eiichi and Emonts, Bjorn and Guillard, Pierre and Helou, George and Lanz, Lauranne and Madden, Susanne and Medling, Anne and O'Sullivan, Ewan and Ogle, Patrick and Pope, Alexandra and Pineau des Forêts, Guillaume and Shull, J. Michael and Smith, John-David and Togi, Aditya and Xu, C. Kevin (2019) Warm H_2 as a probe of massive accretion and feedback through shocks and turbulence across cosmic time. Astro2020 Science White Paper, . (Unpublished) http://resolver.caltech.edu/CaltechAUTHORS:20190626-104726557

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Abstract

Galaxy formation depends on a complex interplay between gravitational collapse, gas accretion, merging, and feedback processes. Yet, after many decades of investigation, these concepts are poorly understood. This paper presents the argument that warm H_2 can be used as a tool to unlock some of these mysteries. Turbulence, shocks and outflows, driven by star formation, AGN activity or inflows, may prevent the rapid buildup of star formation in galaxies. Central to our understanding of how gas is converted into stars is the process by which gas can dissipate its mechanical energy through turbulence and shocks in order to cool. H_2 lines provide direct quantitative measurements of kinetic energy dissipation in molecular gas in galaxies throughout the Universe. Based on the detection of very powerful H_2 lines from z = 2 galaxies and proto-clusters at the detection limits of Spitzer, we are confident that future far-IR and UV H_2 observations will provide a wealth of new information and insight into galaxy evolution to high-z. Finally, at the very earliest epoch of star and galaxy formation, warm H_2 may also provide a unique glimpse of molecular gas collapse at 7 < z < 12 in massive dark matter (DM) halos on their way to forming the very first galaxies. Such measurements are beyond the reach of existing and planned observatories.


Item Type:Report or Paper (White Paper)
Related URLs:
URLURL TypeDescription
http://arxiv.org/abs/1903.06653arXivDiscussion Paper
ORCID:
AuthorORCID
Appleton, Philip N.0000-0002-7607-8766
Armus, Lee0000-0003-3498-2973
Capak, Peter0000-0003-3578-6843
Cluver, Michelle0000-0002-9871-6490
Cooray, Asantha0000-0002-3892-0190
Díaz-Santos, Tanio0000-0003-0699-6083
Helou, George0000-0003-3367-3415
Lanz, Lauranne0000-0002-3249-8224
Medling, Anne0000-0001-7421-2944
Ogle, Patrick0000-0002-3471-981X
Pope, Alexandra0000-0001-8592-2706
Smith, John-David0000-0003-1545-5078
Xu, C. Kevin0000-0002-1588-6700
Series Name:Astro2020 Science White Paper
Record Number:CaltechAUTHORS:20190626-104726557
Persistent URL:http://resolver.caltech.edu/CaltechAUTHORS:20190626-104726557
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:96734
Collection:CaltechAUTHORS
Deposited By: Tony Diaz
Deposited On:26 Jun 2019 17:56
Last Modified:24 Jul 2019 22:24

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