Ly$\alpha$ photons scattered by neutral hydrogen atoms in the circumgalactic
media or produced in the halos of star-forming galaxies are expected to lead to
extended Ly$\alpha$ emission around galaxies. Such low surface brightness
Ly$\alpha$ halos (LAHs) have been detected by stacking Ly$\alpha$ images of
high-redshift star-forming galaxies. We study the origin of LAHs by performing
radiative transfer modeling of nine $z=3.1$ Lyman-Alpha Emitters (LAEs) in a
high resolution hydrodynamic galaxy formation simulation. We develop a method
of computing the mean Ly$\alpha$ surface brightness profile of each LAE by
effectively integrating over many different observing directions. Without
adjusting any parameters, our model yields an average Ly$\alpha$ surface
brightness profile in remarkable agreement with observations. We find that
observed LAHs can not be accounted for solely by photons originating from the
central LAE and scattered to large radii by hydrogen atoms in the
circumgalactic gas. Instead, Ly$\alpha$ emission from regions in the outer halo
is primarily responsible for producing the extended LAHs seen in observations,
which potentially includes both star-forming and cooling radiation. The
contribution from star formation in the outer halo regions can be strongly
constrained to be negligible by the observed absence of an extended
ultra-violet (UV) halo. Our results therefore suggest that cooling radiation
from the outer halo regions of LAEs plays a major role in forming their
extended LAHs. We discuss the implications and caveats of such a picture.
Description
[1502.01349] On the Diffuse Lyman-alpha Halo Around Lyman-alpha Emitting Galaxies
%0 Generic
%1 lake2015diffuse
%A Lake, Ethan
%A Zheng, Zheng
%A Cen, Renyue
%A Sadoun, Raphael
%A Momose, Rieko
%A Ouchi, Masami
%D 2015
%K alpha diffuse halo lyman
%T On the Diffuse Lyman-alpha Halo Around Lyman-alpha Emitting Galaxies
%U http://arxiv.org/abs/1502.01349
%X Ly$\alpha$ photons scattered by neutral hydrogen atoms in the circumgalactic
media or produced in the halos of star-forming galaxies are expected to lead to
extended Ly$\alpha$ emission around galaxies. Such low surface brightness
Ly$\alpha$ halos (LAHs) have been detected by stacking Ly$\alpha$ images of
high-redshift star-forming galaxies. We study the origin of LAHs by performing
radiative transfer modeling of nine $z=3.1$ Lyman-Alpha Emitters (LAEs) in a
high resolution hydrodynamic galaxy formation simulation. We develop a method
of computing the mean Ly$\alpha$ surface brightness profile of each LAE by
effectively integrating over many different observing directions. Without
adjusting any parameters, our model yields an average Ly$\alpha$ surface
brightness profile in remarkable agreement with observations. We find that
observed LAHs can not be accounted for solely by photons originating from the
central LAE and scattered to large radii by hydrogen atoms in the
circumgalactic gas. Instead, Ly$\alpha$ emission from regions in the outer halo
is primarily responsible for producing the extended LAHs seen in observations,
which potentially includes both star-forming and cooling radiation. The
contribution from star formation in the outer halo regions can be strongly
constrained to be negligible by the observed absence of an extended
ultra-violet (UV) halo. Our results therefore suggest that cooling radiation
from the outer halo regions of LAEs plays a major role in forming their
extended LAHs. We discuss the implications and caveats of such a picture.
@misc{lake2015diffuse,
abstract = {Ly$\alpha$ photons scattered by neutral hydrogen atoms in the circumgalactic
media or produced in the halos of star-forming galaxies are expected to lead to
extended Ly$\alpha$ emission around galaxies. Such low surface brightness
Ly$\alpha$ halos (LAHs) have been detected by stacking Ly$\alpha$ images of
high-redshift star-forming galaxies. We study the origin of LAHs by performing
radiative transfer modeling of nine $z=3.1$ Lyman-Alpha Emitters (LAEs) in a
high resolution hydrodynamic galaxy formation simulation. We develop a method
of computing the mean Ly$\alpha$ surface brightness profile of each LAE by
effectively integrating over many different observing directions. Without
adjusting any parameters, our model yields an average Ly$\alpha$ surface
brightness profile in remarkable agreement with observations. We find that
observed LAHs can not be accounted for solely by photons originating from the
central LAE and scattered to large radii by hydrogen atoms in the
circumgalactic gas. Instead, Ly$\alpha$ emission from regions in the outer halo
is primarily responsible for producing the extended LAHs seen in observations,
which potentially includes both star-forming and cooling radiation. The
contribution from star formation in the outer halo regions can be strongly
constrained to be negligible by the observed absence of an extended
ultra-violet (UV) halo. Our results therefore suggest that cooling radiation
from the outer halo regions of LAEs plays a major role in forming their
extended LAHs. We discuss the implications and caveats of such a picture.},
added-at = {2015-02-06T09:55:00.000+0100},
author = {Lake, Ethan and Zheng, Zheng and Cen, Renyue and Sadoun, Raphael and Momose, Rieko and Ouchi, Masami},
biburl = {https://www.bibsonomy.org/bibtex/2312f943c659d353734ff9f17606fde2c/miki},
description = {[1502.01349] On the Diffuse Lyman-alpha Halo Around Lyman-alpha Emitting Galaxies},
interhash = {5f86af69473244afd5eb90f6074adc9b},
intrahash = {312f943c659d353734ff9f17606fde2c},
keywords = {alpha diffuse halo lyman},
note = {cite arxiv:1502.01349Comment: 11 pages, 8 figures, submitted to ApJ},
timestamp = {2015-02-06T09:55:00.000+0100},
title = {On the Diffuse Lyman-alpha Halo Around Lyman-alpha Emitting Galaxies},
url = {http://arxiv.org/abs/1502.01349},
year = 2015
}