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Title: Discovery of a stellar overdensity in Eridanus-Phoenix in the dark energy survey

Journal Article · · The Astrophysical Journal (Online)

Here, we report the discovery of an excess of main sequence turn-off stars in the direction of the constellations of Eridanus and Phoenix from the first year data of the Dark Energy Survey (DES). The Eridanus-Phoenix (EriPhe) overdensity is centered around l ~ 285° and b~-60° and spans at least 30° in longitude and 10 deg in latitude. The Poisson significance of the detection is at least 9 sigma. The stellar population in the overdense region is similar in brightness and color to that of the nearby globular cluster NGC 1261, indicating that the heliocentric distance of EriPhe is about d~16 kpc. The extent of EriPhe in projection is therefore at least ~4 kpc by ~3 kpc. On the sky, this overdensity is located between NGC 1261 and a new stellar stream discovered by DES at a similar heliocentric distance, the so-called Phoenix Stream. Given their similar distance and proximity to each other, it is possible that these three structures may be kinematically associated. Alternatively, the EriPhe overdensity is morphologically similar to the Virgo overdensity and the Hercules-Aquila cloud, which also lie at a similar Galactocentric distance. These three overdensities lie along a polar plane separated by ~120° and may share a common origin. Spectroscopic follow-up observations of the stars in EriPhe are required to fully understand the nature of this overdensity.

Research Organization:
Fermi National Accelerator Lab. (FNAL), Batavia, IL (United States); SLAC National Accelerator Lab., Menlo Park, CA (United States)
Sponsoring Organization:
USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Organization:
The DES Collaboration
Grant/Contract Number:
AC02-07CH11359; AC02-76SF00515
OSTI ID:
1234896
Alternate ID(s):
OSTI ID: 1257727
Report Number(s):
FERMILAB-PUB-15-392-AE; SLAC-PUB-16571; arXiv eprint number arXiv:1509.04296
Journal Information:
The Astrophysical Journal (Online), Vol. 817, Issue 2; ISSN 1538-4357
Publisher:
Institute of Physics (IOP)Copyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 26 works
Citation information provided by
Web of Science

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Cited By (16)

The outer envelopes of globular clusters. II. NGC 1851, NGC 5824 and NGC 1261* journal September 2017
Tails and streams around the Galactic globular clusters NGC 1851, NGC 1904, NGC 2298 and NGC 2808 journal October 2017
Common origin for Hercules-Aquila and Virgo Clouds in Gaia DR2 journal October 2018
Disentangling the Virgo Overdensity with rr Lyrae Stars journal November 2016
Identification of RR Lyrae Stars in Multiband, Sparsely Sampled Data from the Dark Energy Survey Using Template Fitting and Random Forest Classification journal June 2019
Stellar Streams Discovered in the Dark Energy Survey journal July 2018
Proper Motions of Stellar Streams Discovered in the Dark Energy Survey journal October 2019
Triangulum–Andromeda Overdensity: a Region with a Complex Stellar Population journal November 2019
The Virgo Overdensity Explained journal November 2019
Fitting the Density Substructure of the Stellar Halo with MilkyWay@home journal September 2018
Disentangling the Virgo Overdensity with RR Lyrae stars text January 2016
The Outer Envelopes of Globular Clusters. II. NGC 1851, NGC 5824 and NGC 1261 text January 2017
Common origin for Hercules-Aquila and Virgo Clouds in Gaia DR2 text January 2018
Fitting the density substructure of the stellar halo with MilkyWay@home text January 2018
Identification of RR Lyrae stars in multiband, sparsely-sampled data from the Dark Energy Survey using template fitting and Random Forest classification text January 2019
Triangulum-Andromeda overdensity: a region with a complex stellar population text January 2019

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