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Title: Farthest neighbor: The distant Milky Way satellite Eridanus II

Abstract

We present Magellan/IMACS spectroscopy of the recently-discovered Milky Way satellite Eridanus II (Eri II). We identify 28 member stars in Eri II, from which we measure a systemic radial velocity of $$v_{\rm hel} = 75.6 \pm 1.3~\mbox{(stat.)} \pm 2.0~\mbox{(sys.)}~\mathrm{km\,s^{-1}}$$ and a velocity dispersion of $$6.9^{+1.2}_{-0.9}~\mathrm{km\,s^{-1}}$$. Assuming that Eri~II is a dispersion-supported system in dynamical equilibrium, we derive a mass within the half-light radius of Eri II is $$1.2^{+0.4}_{-0.3} \times 10^{7}~\mathrm{M_\odot}$$, indicating a mass-to-light ratio of $$420^{+210}_{-140}~\mathrm{M_\odot}/\mathrm{L_\odot}$$ and confirming that it is a dark matter-dominated dwarf galaxy. From the equivalent width measurements of the CaT lines of 16 red giant member stars, we derive a mean metallicity of $${\rm [Fe/H]} = -2.38 \pm 0.13$$ and a metallicity dispersion of $$\sigma_{\rm [Fe/H]} = 0.47 ^{+0.12}_{-0.09}$$. The velocity of Eri II in the Galactic Standard of Rest frame is $$v_{\rm GSR} = -66.6~\mathrm{km\,s^{-1}}$$, indicating that either Eri II is falling into the Milky Way potential for the first time or it has passed the apocenter of its orbit on a subsequent passage. At a Galactocentric distance of $$\sim$$370 kpc, Eri II is one of the Milky Way's most distant satellites known. Additionally, we show that the bright blue stars previously suggested to be a young stellar population are not associated with Eri II. The lack of gas and recent star formation in Eri II is surprising given its mass and distance from the Milky Way, and may place constraints on models of quenching in dwarf galaxies and on the distribution of hot gas in the Milky Way halo. Furthermore, the large velocity dispersion of Eri II can be combined with the existence of a central star cluster to constrain MACHO dark matter with mass $$\gtrsim10~\mathrm{M_\odot}$$.

Authors:
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Publication Date:
Research Org.:
Oak Ridge National Laboratory (ORNL), Oak Ridge, TN (United States); Lawrence Berkeley National Laboratory (LBNL), Berkeley, CA (United States); SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States); Fermi National Accelerator Laboratory (FNAL), Batavia, IL (United States)
Sponsoring Org.:
USDOE Office of Science (SC), High Energy Physics (HEP)
Contributing Org.:
DES Collaboration
OSTI Identifier:
1349627
Alternate Identifier(s):
OSTI ID: 1345629; OSTI ID: 1368580
Report Number(s):
FERMILAB-PUB-16-479-AE-PPD; arXiv:1611.05052
Journal ID: ISSN 1538-4357; KJ0402000; KJ0503000; ERKJ311; ERKJEPM; TRN: US1700601
Grant/Contract Number:  
AC05-00OR22725; AC02-07CH11359; AC02-76SF00515
Resource Type:
Accepted Manuscript
Journal Name:
The Astrophysical Journal (Online)
Additional Journal Information:
Journal Name: The Astrophysical Journal (Online); Journal Volume: 838; Journal Issue: 1; Journal ID: ISSN 1538-4357
Publisher:
Institute of Physics (IOP)
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; dark matter; galaxies: dwarf; galaxies: individual (Eridanus II); galaxies: stellar content; Local Group; stars: abundances

Citation Formats

Li, T. S., Simon, J. D., Drlica-Wagner, A., Bechtol, K., Wang, M. Y., García-Bellido, J., Frieman, J., Marshall, J. L., James, D. J., Strigari, L., Pace, A. B., Balbinot, E., Zhang, Y., Abbott, T. M. C., Allam, S., Benoit-Lévy, A., Bernstein, G. M., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cunha, C. E., D’Andrea, C. B., Costa, L. N. da, DePoy, D. L., Desai, S., Diehl, H. T., Eifler, T. F., Flaugher, B., Goldstein, D. A., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Krause, E., Kuehn, K., Lin, H., Maia, M. A. G., March, M., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Santiago, B., Schubnell, M., Sevilla-Noarbe, I., Smith, R. C., Sobreira, F., Suchyta, E., Tarle, G., Thomas, D., Tucker, D. L., Walker, A. R., Wechsler, R. H., Wester, W., and Yanny, B. Farthest neighbor: The distant Milky Way satellite Eridanus II. United States: N. p., 2017. Web. doi:10.3847/1538-4357/aa6113.
Li, T. S., Simon, J. D., Drlica-Wagner, A., Bechtol, K., Wang, M. Y., García-Bellido, J., Frieman, J., Marshall, J. L., James, D. J., Strigari, L., Pace, A. B., Balbinot, E., Zhang, Y., Abbott, T. M. C., Allam, S., Benoit-Lévy, A., Bernstein, G. M., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cunha, C. E., D’Andrea, C. B., Costa, L. N. da, DePoy, D. L., Desai, S., Diehl, H. T., Eifler, T. F., Flaugher, B., Goldstein, D. A., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Krause, E., Kuehn, K., Lin, H., Maia, M. A. G., March, M., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Santiago, B., Schubnell, M., Sevilla-Noarbe, I., Smith, R. C., Sobreira, F., Suchyta, E., Tarle, G., Thomas, D., Tucker, D. L., Walker, A. R., Wechsler, R. H., Wester, W., & Yanny, B. Farthest neighbor: The distant Milky Way satellite Eridanus II. United States. https://doi.org/10.3847/1538-4357/aa6113
Li, T. S., Simon, J. D., Drlica-Wagner, A., Bechtol, K., Wang, M. Y., García-Bellido, J., Frieman, J., Marshall, J. L., James, D. J., Strigari, L., Pace, A. B., Balbinot, E., Zhang, Y., Abbott, T. M. C., Allam, S., Benoit-Lévy, A., Bernstein, G. M., Bertin, E., Brooks, D., Burke, D. L., Rosell, A. Carnero, Kind, M. Carrasco, Carretero, J., Cunha, C. E., D’Andrea, C. B., Costa, L. N. da, DePoy, D. L., Desai, S., Diehl, H. T., Eifler, T. F., Flaugher, B., Goldstein, D. A., Gruen, D., Gruendl, R. A., Gschwend, J., Gutierrez, G., Krause, E., Kuehn, K., Lin, H., Maia, M. A. G., March, M., Menanteau, F., Miquel, R., Plazas, A. A., Romer, A. K., Sanchez, E., Santiago, B., Schubnell, M., Sevilla-Noarbe, I., Smith, R. C., Sobreira, F., Suchyta, E., Tarle, G., Thomas, D., Tucker, D. L., Walker, A. R., Wechsler, R. H., Wester, W., and Yanny, B. Fri . "Farthest neighbor: The distant Milky Way satellite Eridanus II". United States. https://doi.org/10.3847/1538-4357/aa6113. https://www.osti.gov/servlets/purl/1349627.
@article{osti_1349627,
title = {Farthest neighbor: The distant Milky Way satellite Eridanus II},
author = {Li, T. S. and Simon, J. D. and Drlica-Wagner, A. and Bechtol, K. and Wang, M. Y. and García-Bellido, J. and Frieman, J. and Marshall, J. L. and James, D. J. and Strigari, L. and Pace, A. B. and Balbinot, E. and Zhang, Y. and Abbott, T. M. C. and Allam, S. and Benoit-Lévy, A. and Bernstein, G. M. and Bertin, E. and Brooks, D. and Burke, D. L. and Rosell, A. Carnero and Kind, M. Carrasco and Carretero, J. and Cunha, C. E. and D’Andrea, C. B. and Costa, L. N. da and DePoy, D. L. and Desai, S. and Diehl, H. T. and Eifler, T. F. and Flaugher, B. and Goldstein, D. A. and Gruen, D. and Gruendl, R. A. and Gschwend, J. and Gutierrez, G. and Krause, E. and Kuehn, K. and Lin, H. and Maia, M. A. G. and March, M. and Menanteau, F. and Miquel, R. and Plazas, A. A. and Romer, A. K. and Sanchez, E. and Santiago, B. and Schubnell, M. and Sevilla-Noarbe, I. and Smith, R. C. and Sobreira, F. and Suchyta, E. and Tarle, G. and Thomas, D. and Tucker, D. L. and Walker, A. R. and Wechsler, R. H. and Wester, W. and Yanny, B.},
abstractNote = {We present Magellan/IMACS spectroscopy of the recently-discovered Milky Way satellite Eridanus II (Eri II). We identify 28 member stars in Eri II, from which we measure a systemic radial velocity of $v_{\rm hel} = 75.6 \pm 1.3~\mbox{(stat.)} \pm 2.0~\mbox{(sys.)}~\mathrm{km\,s^{-1}}$ and a velocity dispersion of $6.9^{+1.2}_{-0.9}~\mathrm{km\,s^{-1}}$. Assuming that Eri~II is a dispersion-supported system in dynamical equilibrium, we derive a mass within the half-light radius of Eri II is $1.2^{+0.4}_{-0.3} \times 10^{7}~\mathrm{M_\odot}$, indicating a mass-to-light ratio of $420^{+210}_{-140}~\mathrm{M_\odot}/\mathrm{L_\odot}$ and confirming that it is a dark matter-dominated dwarf galaxy. From the equivalent width measurements of the CaT lines of 16 red giant member stars, we derive a mean metallicity of ${\rm [Fe/H]} = -2.38 \pm 0.13$ and a metallicity dispersion of $\sigma_{\rm [Fe/H]} = 0.47 ^{+0.12}_{-0.09}$. The velocity of Eri II in the Galactic Standard of Rest frame is $v_{\rm GSR} = -66.6~\mathrm{km\,s^{-1}}$, indicating that either Eri II is falling into the Milky Way potential for the first time or it has passed the apocenter of its orbit on a subsequent passage. At a Galactocentric distance of $\sim$370 kpc, Eri II is one of the Milky Way's most distant satellites known. Additionally, we show that the bright blue stars previously suggested to be a young stellar population are not associated with Eri II. The lack of gas and recent star formation in Eri II is surprising given its mass and distance from the Milky Way, and may place constraints on models of quenching in dwarf galaxies and on the distribution of hot gas in the Milky Way halo. Furthermore, the large velocity dispersion of Eri II can be combined with the existence of a central star cluster to constrain MACHO dark matter with mass $\gtrsim10~\mathrm{M_\odot}$.},
doi = {10.3847/1538-4357/aa6113},
journal = {The Astrophysical Journal (Online)},
number = 1,
volume = 838,
place = {United States},
year = {Fri Mar 17 00:00:00 EDT 2017},
month = {Fri Mar 17 00:00:00 EDT 2017}
}

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Rapid Environmental Quenching of Satellite Dwarf Galaxies in the Local Group
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Sweating the small stuff: simulating dwarf galaxies, ultra-faint dwarf galaxies, and their own tiny satellites
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Synthesis of RKA 182
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Two major accretion epochs in M31 from two distinct populations of globular clusters.
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Pre-launch estimates for GLAST sensitivity to Dark Matter annihilation signals
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On the Reported Death of the MACHO Era
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Local Kinematics and the Local Standard of Rest
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A Complete Spectroscopic Survey of the Milky Way Satellite Segue 1: The Darkest Galaxy
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The Hercules satellite: a stellar stream in the Milky Way halo?
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Dwarf Galaxy Dark Matter Density Profiles Inferred from Stellar and Gas Kinematics
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Dwarf galaxy annihilation and decay emission profiles for dark matter experiments
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Search for Gamma-Ray Emission from DES Dwarf Spheroidal Galaxy Candidates with Fermi-LAT Data
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A New Faint Milky Way Satellite Discovered in the Pan-STARRS1 3 pi Survey
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Hydra II: a faint and compact Milky Way dwarf galaxy found in the Survey of the Magellanic Stellar History
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Taking Care of Business in a Flash: Constraining the Timescale for Low-Mass Satellite Quenching with ELVIS
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Stellar Kinematics and Metallicities in the Ultra-Faint Dwarf Galaxy Reticulum II
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Eight Ultra-faint Galaxy Candidates Discovered in Year Two of the Dark Energy Survey
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The Galaxy in Context: Structural, Kinematic and Integrated Properties
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A New Milky Way Satellite Discovered In The Subaru/Hyper Suprime-Cam Survey
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New Understanding of Large Magellanic Cloud Structure, Dynamics and Orbit from Carbon Star Kinematics
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The Structure of Cold Dark Matter Halos
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Improved constraints from ultra-faint dwarf galaxies on primordial black holes as dark matter
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Extending the globular cluster system–halo mass relation to the lowest galaxy masses
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The suppression of star formation on the smallest scales: what role does environment play?
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Too big to fail in light of Gaia
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Evidence of a Non-universal Stellar Initial Mass Function. Insights from HST Optical Imaging of Six Ultra-faint Dwarf Milky Way Satellites
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The Missing Satellites of the Magellanic Clouds? Gaia Proper Motions of the Recently Discovered Ultra-faint Galaxies
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Proper Motions of Milky Way Ultra-faint Satellites with Gaia DR2 × DES DR1
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The hidden giant: Discovery of an enormous Galactic dwarf satellite in Gaia DR2
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Chemical Abundance Analysis of Three α -poor, Metal-poor Stars in the Ultrafaint Dwarf Galaxy Horologium I
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Searching for Primordial Black Holes in the radio and X-ray sky
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Dynamics of dwarf galaxies disfavor stellar-mass black hole dark matter
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CMB bounds on disk-accreting massive Primordial Black Holes
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Dynamical Histories of the Crater II and Hercules Dwarf Galaxies
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