An extended cold gas absorber in a central cluster galaxy
R. Smith, and A. Edge. (2017)cite arxiv:1706.08533Comment: MNRAS Letters, accepted.
Abstract
We present the serendipitous discovery of an extended cold gas structure
projected close to the brightest cluster galaxy (BCG) of the z=0.045 cluster
Abell 3716, from archival integral field spectroscopy. The gas is revealed
through narrow Na D line absorption, seen against the stellar light of the BCG,
which can be traced for $\sim$25 kpc, with a width of 2-4 kpc. The gas is
offset to higher velocity than the BCG (by $\sim$100 km/s), showing that it is
infalling rather than outflowing; the intrinsic linewidth is $\sim$80 km/s
(FWHM). Very weak H$\alpha$ line emission is detected from the structure, and a
weak dust absorption feature is suggested from optical imaging, but no stellar
counterpart has been identified. We discuss some possible interpretations for
the absorber: as a projected low-surface-brightness galaxy, as a stream of gas
that was stripped from an infalling cluster galaxy, or as a "retired" cool-core
nebula filament.
Description
[1706.08533] An extended cold gas absorber in a central cluster galaxy
%0 Generic
%1 smith2017extended
%A Smith, Russell J.
%A Edge, Alastair C.
%D 2017
%K absorption cluster extended filament
%T An extended cold gas absorber in a central cluster galaxy
%U http://arxiv.org/abs/1706.08533
%X We present the serendipitous discovery of an extended cold gas structure
projected close to the brightest cluster galaxy (BCG) of the z=0.045 cluster
Abell 3716, from archival integral field spectroscopy. The gas is revealed
through narrow Na D line absorption, seen against the stellar light of the BCG,
which can be traced for $\sim$25 kpc, with a width of 2-4 kpc. The gas is
offset to higher velocity than the BCG (by $\sim$100 km/s), showing that it is
infalling rather than outflowing; the intrinsic linewidth is $\sim$80 km/s
(FWHM). Very weak H$\alpha$ line emission is detected from the structure, and a
weak dust absorption feature is suggested from optical imaging, but no stellar
counterpart has been identified. We discuss some possible interpretations for
the absorber: as a projected low-surface-brightness galaxy, as a stream of gas
that was stripped from an infalling cluster galaxy, or as a "retired" cool-core
nebula filament.
@misc{smith2017extended,
abstract = {We present the serendipitous discovery of an extended cold gas structure
projected close to the brightest cluster galaxy (BCG) of the z=0.045 cluster
Abell 3716, from archival integral field spectroscopy. The gas is revealed
through narrow Na D line absorption, seen against the stellar light of the BCG,
which can be traced for $\sim$25 kpc, with a width of 2-4 kpc. The gas is
offset to higher velocity than the BCG (by $\sim$100 km/s), showing that it is
infalling rather than outflowing; the intrinsic linewidth is $\sim$80 km/s
(FWHM). Very weak H$\alpha$ line emission is detected from the structure, and a
weak dust absorption feature is suggested from optical imaging, but no stellar
counterpart has been identified. We discuss some possible interpretations for
the absorber: as a projected low-surface-brightness galaxy, as a stream of gas
that was stripped from an infalling cluster galaxy, or as a "retired" cool-core
nebula filament.},
added-at = {2017-06-28T06:56:33.000+0200},
author = {Smith, Russell J. and Edge, Alastair C.},
biburl = {https://www.bibsonomy.org/bibtex/26ba15fb38a633999d7f698617bc6945a/miki},
description = {[1706.08533] An extended cold gas absorber in a central cluster galaxy},
interhash = {5725e0fdb8f1519f857b223d28c71d95},
intrahash = {6ba15fb38a633999d7f698617bc6945a},
keywords = {absorption cluster extended filament},
note = {cite arxiv:1706.08533Comment: MNRAS Letters, accepted},
timestamp = {2017-06-28T06:56:33.000+0200},
title = {An extended cold gas absorber in a central cluster galaxy},
url = {http://arxiv.org/abs/1706.08533},
year = 2017
}