We present the discovery of compact, obscured star formation in galaxies at z
0.6 that exhibit >1000 km/s outflows. Using optical morphologies from the
Hubble Space Telescope and infrared photometry from the Wide-field Infrared
Survey Explorer, we estimate star formation rate (SFR) surface densities that
approach Sigma_SFR 3000 Msun/yr/kpc^2, comparable to the Eddington limit from
radiation pressure on dust grains. We argue that feedback associated with a
compact starburst in the form of radiation pressure from massive stars and ram
pressure from supernovae and stellar winds is sufficient to produce the
high-velocity outflows we observe, without the need to invoke feedback from an
active galactic nucleus.
Description
[1205.2368] High-Velocity Outflows Without AGN Feedback: Eddington-Limited Star Formation in Compact Massive Galaxies
%0 Generic
%1 diamondstanic2012highvelocity
%A Diamond-Stanic, Aleksandar M.
%A Moustakas, John
%A Tremonti, Christy A.
%A Coil, Alison L.
%A Hickox, Ryan C.
%A Robaina, Aday R.
%A Rudnick, Gregory H.
%A Sell, Paul H.
%D 2012
%K eddington limit sfr wind
%T High-Velocity Outflows Without AGN Feedback: Eddington-Limited Star
Formation in Compact Massive Galaxies
%U http://arxiv.org/abs/1205.2368
%X We present the discovery of compact, obscured star formation in galaxies at z
0.6 that exhibit >1000 km/s outflows. Using optical morphologies from the
Hubble Space Telescope and infrared photometry from the Wide-field Infrared
Survey Explorer, we estimate star formation rate (SFR) surface densities that
approach Sigma_SFR 3000 Msun/yr/kpc^2, comparable to the Eddington limit from
radiation pressure on dust grains. We argue that feedback associated with a
compact starburst in the form of radiation pressure from massive stars and ram
pressure from supernovae and stellar winds is sufficient to produce the
high-velocity outflows we observe, without the need to invoke feedback from an
active galactic nucleus.
@misc{diamondstanic2012highvelocity,
abstract = {We present the discovery of compact, obscured star formation in galaxies at z
0.6 that exhibit >1000 km/s outflows. Using optical morphologies from the
Hubble Space Telescope and infrared photometry from the Wide-field Infrared
Survey Explorer, we estimate star formation rate (SFR) surface densities that
approach Sigma_SFR 3000 Msun/yr/kpc^2, comparable to the Eddington limit from
radiation pressure on dust grains. We argue that feedback associated with a
compact starburst in the form of radiation pressure from massive stars and ram
pressure from supernovae and stellar winds is sufficient to produce the
high-velocity outflows we observe, without the need to invoke feedback from an
active galactic nucleus.},
added-at = {2012-05-14T03:02:49.000+0200},
author = {Diamond-Stanic, Aleksandar M. and Moustakas, John and Tremonti, Christy A. and Coil, Alison L. and Hickox, Ryan C. and Robaina, Aday R. and Rudnick, Gregory H. and Sell, Paul H.},
biburl = {https://www.bibsonomy.org/bibtex/20611008c0606e55fdcb3b991e2e838b5/miki},
description = {[1205.2368] High-Velocity Outflows Without AGN Feedback: Eddington-Limited Star Formation in Compact Massive Galaxies},
interhash = {ca7e4a770f8c3215dbc0c18146c9184e},
intrahash = {0611008c0606e55fdcb3b991e2e838b5},
keywords = {eddington limit sfr wind},
note = {cite arxiv:1205.2368Comment: 6 pages, 4 figures, submitted to ApJ Letters},
timestamp = {2012-05-14T03:02:49.000+0200},
title = {High-Velocity Outflows Without AGN Feedback: Eddington-Limited Star
Formation in Compact Massive Galaxies},
url = {http://arxiv.org/abs/1205.2368},
year = 2012
}