: The destruction of a bright dwarf galaxy as revealed by the chemistry of the Indus stellar stream
arXiv:2104.13883 · doi:10.3847/1538-4357/abfc54
Abstract
The recently discovered Indus stellar stream exhibits a diverse chemical signature compared to what is found for most other streams due to the abundances of two outlier stars, Indus0 and Indus13. Indus13, exhibits an extreme enhancement in rapid neutron-capture (-)process elements with . It thus provides direct evidence of the accreted nature of -process enhanced stars. In this paper we present a detailed chemical analysis of the neutron-capture elements in Indus13, revealing the star to be slightly actinide poor. The other outlier, Indus, displays a globular cluster-like signature with high N, Na, and Al abundances, while the rest of the Indus stars show abundances compatible with a dwarf galaxy origin. Hence, Indus provides the first chemical evidence of a fully disrupted dwarf containing a globular cluster. We use the chemical signature of the Indus stars to discuss the nature of the stream progenitor which was likely a chemically evolved system, with a mass somewhere in the range from Ursa Minor to Fornax.
14 pages, 4 figures, and 5 tables, accepted for publication in ApJ
References in corpus (43)
- The NumPy array: a structure for efficient numerical computation
- The Gaia mission
- The Dartmouth Stellar Evolution Database
- Light Curves of the Neutron Star Merger GW170817/SSS17a: Implications for R-Process Nucleosynthesis
- Magnetorotationally driven Supernovae as the origin of early galaxy -process elements?
- Beasts of the Southern Wild: Discovery of nine Ultra Faint satellites in the vicinity of the Magellanic Clouds
- CH in stellar atmospheres: an extensive linelist
- What is a globular cluster? An observational perspective
- Near-UV Observations of HD221170: New Insights into the Nature of r-Process-Rich Stars
- A high resolution VLT/FLAMES study of individual stars in the centre of the Fornax dwarf spheroidal galaxy
- The Chemical Evolution of the Draco Dwarf Spheroidal Galaxy
- New Rare Earth Element Abundance Distributions for the Sun and Five r-Process-Rich Very Metal-Poor Stars
- Multi-Element Abundance Measurements from Medium-Resolution Spectra. IV. Alpha Element Distributions in Milky Way Dwarf Satellite Galaxies
- Improved Laboratory Transition Probabilities for Ce II, Application to the Cerium Abundances of the Sun and Five r-process Rich, Metal-Poor Stars, and Rare Earth Lab Data
- Dynamical Relics of the Ancient Galactic Halo
- VLT/UVES Spectroscopy of Individual Stars in Three Globular Clusters in the Fornax Dwarf Spheroidal Galaxy
- Non-LTE aluminium abundances in late-type stars
- An R-process enhanced star in the dwarf galaxy Tucana III
- The -Process Alliance: Fourth Data Release from the Search for -Process-Enhanced Stars in the Galactic Halo
- Improved Laboratory Transition Probabilities for Er II and Applications to the Erbium Abundances of the Sun and Five r-Process Rich, Metal-Poor Stars
- Multiple populations in globular clusters and their parent galaxies
- VLT/FLAMES spectroscopy of red giant branch stars in the Fornax dwarf spheroidal galaxy
- The R-process Alliance: First Magellan/MIKE Release from the Southern Search for R-Process-enhanced Stars
- The Southern Stellar Stream Spectroscopic Survey (S5): Chemical Abundances of Seven Stellar Streams
- Elevated r-process enrichment in Gaia Sausage and Sequoia
- Nitrogen abundances and multiple stellar populations in the globular clusters of the Fornax dSph
- The Hamburg/ESO R-process Enhanced Star survey (HERES) X. HE 2252-4225, one more r-process enhanced and actinide-boost halo star
- Detailed Abundances of Two Very Metal-Poor Stars in Dwarf Galaxies
- Dynamically Tagged Groups of Very Metal-poor Halo Stars from the HK and Hamburg/ESO Surveys
- An old, metal-poor globular cluster in Sextans A and the metallicity floor of globular cluster systems
- The R-Process Alliance: Chemo-Dynamically Tagged Groups of Halo -Process-Enhanced Stars Reveal a Shared Chemical-Evolution History
- The Populations of Carina. II. Chemical Enrichment
- The role of cluster mass in the multiple populations of Galactic and extragalactic globular clusters
- The Milky Way's stellar streams and globular clusters do not align in a Vast Polar Structure
- Chemical Analysis of the Ultra-Faint Dwarf Galaxy Grus~II. Signature of high-mass stellar nucleosynthesis
- R-process-rich stellar streams in the Milky Way
- Search for globular clusters associated with the Milky Way dwarf galaxies using Gaia DR2
- The GALAH Survey: Chemically tagging the Fimbulthul stream to the globular cluster Centauri
- Rediscovery of the Sixth Star Cluster in the Fornax Dwarf Spheroidal Galaxy
- A chemo-dynamical link between the Gjöll stream and NGC 3201
- Extreme r-process enhanced stars at high metallicity in Fornax
- Detection of Pb II in the Ultraviolet Spectra of Three Metal-Poor Stars
- An investigation of C, N and Na abundances in red giant stars of the Sculptor dwarf spheroidal galaxy
Cited by in corpus (8)
- Origin of highly -process-enhanced stars in a cosmological zoom-in simulation of a Milky Way-like galaxy
- Extending the Chemical Reach of the H3 Survey: Detailed Abundances of the Dwarf-galaxy Stellar Stream Wukong/LMS-1
- Potential Black Hole Seeding of the Spiral Galaxy NGC 4424 via an Infalling Star Cluster
- Finding -II sibling stars in the Milky Way with the Greedy Optimistic Clustering algorithm
- Chemical Abundances of the Typhon Stellar Stream
- Discovery of a pair of very metal-poor stars enriched in neutron-capture elements: The proto-disk r-II star BPS CS 29529-0089 and the Gaia-Sausage-Enceladus r-I star TYC 9219-2422-1
- Detection of the actinide Th in an r-process-enhanced star with accretion origin
- Epicyclic Density Variations in the Indus Stellar Stream