2016/04/30 by Denija Crnojević, D. Crnojević, D. J. Sand +9 · 118 citations
Physics and Astronomy · Psychology · #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Cluster (spacecraft) #Computer science #Gamma-ray bursts and supernovae #Operating system #Physics #Psychology #Star (game theory) #Stellar, planetary, and galactic studies #astro-ph.GA
paper · pdf · doi:10.3847/2041-8205/824/1/l14
published in The Astrophysical Journal Letters 824(1), L14 (IOP Publishing) · 7 pages, 4 figures; ApJL accepted
arxiv created 2016/05/27 · openalex publication_date 2016/06/08 · arxiv updated 2016/06/15 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
ABSTRACT We present deep imaging of the most distant dwarf discovered by the Dark Energy Survey, Eridanus II (Eri II). Our Magellan /Megacam stellar photometry reaches ∼3 mag deeper than previous work and allows us to confirm the presence of a stellar cluster whose position is consistent with Eri II’s center. This makes Eri II, at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>V</mml:mi> </mml:mrow> </mml:msub> <mml:mo>=</mml:mo> <mml:mo>−</mml:mo> <mml:mn>7.1</mml:mn> </mml:math> , the least luminous galaxy known to host a (possibly central) cluster. The cluster is partially resolved, and at <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" overflow="scroll"> <mml:msub> <mml:mrow> <mml:mi>M</mml:mi> </mml:mrow> <mml:mrow> <mml:mi>V</mml:mi> </mml:mrow> </mml:msub> <mml:mo>=</mml:mo> <mml:mo>−</mml:mo> <mml:mn>3.5</mml:mn> </mml:math> it accounts for ∼4% of Eri II’s luminosity. We derive updated structural parameters for Eri II, which has a half-light radius of ∼280 pc and is elongated ( ϵ ∼ 0.48) at a measured distance of D ∼ 370 kpc. The color–magnitude diagram displays a blue, extended horizontal branch, as well as a less populated red horizontal branch. A central concentration of stars brighter than the old main-sequence turnoff hints at a possible intermediate-age (∼3 Gyr) population; alternatively, these sources could be blue straggler stars. A deep Green Bank Telescope observation of Eri II reveals no associated atomic gas.