We report the discovery of an object near M87 in the Virgo Cluster with an
extraordinary blueshift of -1025 km/s, offset from the systemic velocity by
>2300 km/s. Evaluation of photometric and spectroscopic data provides strong
evidence that this object is a distant massive globular cluster, which we call
HVGC-1 in analogy to Galactic hypervelocity stars. We consider but disfavor
more exotic interpretations, such as a system of stars bound to a recoiling
black hole. The odds of observing an outlier as extreme as HVGC-1 in a
virialized distribution of intracluster objects are small; it appears more
likely that the cluster was (or is being) ejected from Virgo following a
three-body interaction. The nature of the interaction is unclear, and could
involve either a subhalo or a binary supermassive black hole at the center of
M87.
Description
[1402.6319] A Globular Cluster Toward M87 with a Radial Velocity < -1000 km/s: The First Hypervelocity Cluster
%0 Generic
%1 caldwell2014globular
%A Caldwell, Nelson
%A Strader, Jay
%A Romanowsky, Aaron J.
%A Brodie, Jean P.
%A Moore, Ben
%A Diemand, Jurg
%A Martizzi, Davide
%D 2014
%K cluster globular high-velocity virgo
%T A Globular Cluster Toward M87 with a Radial Velocity < -1000 km/s: The
First Hypervelocity Cluster
%U http://arxiv.org/abs/1402.6319
%X We report the discovery of an object near M87 in the Virgo Cluster with an
extraordinary blueshift of -1025 km/s, offset from the systemic velocity by
>2300 km/s. Evaluation of photometric and spectroscopic data provides strong
evidence that this object is a distant massive globular cluster, which we call
HVGC-1 in analogy to Galactic hypervelocity stars. We consider but disfavor
more exotic interpretations, such as a system of stars bound to a recoiling
black hole. The odds of observing an outlier as extreme as HVGC-1 in a
virialized distribution of intracluster objects are small; it appears more
likely that the cluster was (or is being) ejected from Virgo following a
three-body interaction. The nature of the interaction is unclear, and could
involve either a subhalo or a binary supermassive black hole at the center of
M87.
@misc{caldwell2014globular,
abstract = {We report the discovery of an object near M87 in the Virgo Cluster with an
extraordinary blueshift of -1025 km/s, offset from the systemic velocity by
>2300 km/s. Evaluation of photometric and spectroscopic data provides strong
evidence that this object is a distant massive globular cluster, which we call
HVGC-1 in analogy to Galactic hypervelocity stars. We consider but disfavor
more exotic interpretations, such as a system of stars bound to a recoiling
black hole. The odds of observing an outlier as extreme as HVGC-1 in a
virialized distribution of intracluster objects are small; it appears more
likely that the cluster was (or is being) ejected from Virgo following a
three-body interaction. The nature of the interaction is unclear, and could
involve either a subhalo or a binary supermassive black hole at the center of
M87.},
added-at = {2014-02-27T08:25:48.000+0100},
author = {Caldwell, Nelson and Strader, Jay and Romanowsky, Aaron J. and Brodie, Jean P. and Moore, Ben and Diemand, Jurg and Martizzi, Davide},
biburl = {https://www.bibsonomy.org/bibtex/2c5b0ef0bb86d127a6ddd03c4c1725a84/miki},
description = {[1402.6319] A Globular Cluster Toward M87 with a Radial Velocity < -1000 km/s: The First Hypervelocity Cluster},
interhash = {796bfa0e20c920739fabb25474be9172},
intrahash = {c5b0ef0bb86d127a6ddd03c4c1725a84},
keywords = {cluster globular high-velocity virgo},
note = {cite arxiv:1402.6319Comment: submitted to ApJL, comments welcome},
timestamp = {2014-02-27T08:25:48.000+0100},
title = {A Globular Cluster Toward M87 with a Radial Velocity < -1000 km/s: The
First Hypervelocity Cluster},
url = {http://arxiv.org/abs/1402.6319},
year = 2014
}