An r-process Enhanced Star in the Dwarf Galaxy Tucana III

被引:98
作者
Hansen, T. T. [1 ]
Simon, J. D. [1 ]
Marshall, J. L. [2 ,3 ]
Li, T. S. [2 ,3 ,4 ]
Carollo, D. [5 ,6 ]
DePoy, D. L. [2 ,3 ]
Nagasawa, D. Q. [2 ,3 ]
Bernstein, R. A. [1 ]
Drlica-Wagner, A. [4 ]
Abdalla, F. B. [7 ,8 ]
Allam, S. [4 ]
Annis, J. [4 ]
Bechtol, K. [9 ]
Benoit-Levy, A. [10 ,11 ]
Brooks, D. [7 ]
Buckley-Geer, E. [4 ]
Carnero Rosell, A. [12 ,13 ]
Kind, M. Carrasco [14 ,15 ]
Carretero, J. [16 ,17 ]
Cunha, C. E. [18 ]
da Costa, L. N. [12 ,13 ]
Desai, S. [19 ]
Eifler, T. F. [20 ]
Fausti Neto, A. [12 ]
Flaugher, B. [4 ]
Frieman, J. [21 ]
Garcia-Bellido, J. [22 ]
Gaztanaga, E. [16 ]
Gerdes, D. W. [23 ]
Gruen, D. [18 ,24 ]
Gruendl, R. A. [14 ,15 ]
Gschwend, J. [12 ,13 ]
Gutierrez, G. [4 ]
James, D. J. [25 ,26 ]
Krause, E. [18 ]
Kuehn, K. [27 ]
Kuropatkin, N.
Lahav, O. [7 ]
Miquel, R. [17 ,28 ]
Plazas, A. A. [20 ]
Romer, A. K. [29 ]
Sanchez, E. [30 ]
Santiago, B. [12 ,31 ]
Scarpine, V. [4 ]
Smith, R. C. [26 ]
Soares-Santos, M. [4 ]
Sobreira, F. [12 ,32 ]
Suchyta, E. [33 ]
Swanson, M. E. C. [15 ]
Tarle, G. [23 ]
机构
[1] Observ Carnegie Inst Washington, 813 Santa Barbara St, Pasadena, CA 91101 USA
[2] Texas A&M Univ, George P & Cynthia Woods Mitchell Inst Fundamenta, College Stn, TX 77843 USA
[3] Texas A&M Univ, Dept Phys & Astron, College Stn, TX 77843 USA
[4] Fermilab Natl Accelerator Lab, POB 500, Batavia, IL 60510 USA
[5] Osserv Astron Torino, INAF, Str Osservatorio 20, I-10020 Pino Torinese, Italy
[6] ARC Ctr Excellence All Sky Astrophys CAASTRO, Sydney, NSW, Australia
[7] UCL, Dept Phys & Astron, Gower St, London WC1E 6BT, England
[8] Rhodes Univ, Dept Phys & Elect, POB 94, ZA-6140 Grahamstown, South Africa
[9] LSST, 933 North Cherry Ave, Tucson, AZ 85721 USA
[10] CNRS, Inst Astrophys Paris, UMR 7095, F-75014 Paris, France
[11] UPMC Univ Paris 06, Sorbonne Univ, UMR 7095, Inst Astrophys Paris, F-75014 Paris, France
[12] Lab Interinst E Astron LIneA, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil
[13] Observ Nacl, Rua Gal Jose Cristino 77, BR-20921400 Rio De Janeiro, RJ, Brazil
[14] Univ Illinois, Dept Astron, 1002 W Green St, Urbana, IL 61801 USA
[15] Natl Ctr Supercomp Applicat, 1205 West Clark St, Urbana, IL 61801 USA
[16] IEEC CSIC, Inst Ciencies Espai, Campus UAB,Carrer Can Magrans S-N, E-08193 Barcelona, Spain
[17] Barcelona Inst Sci & Technol, Inst Fis Altes Energies, Campus UAB, E-08193 Barcelona, Spain
[18] Stanford Univ, Kavli Inst Particle Astrophys & Cosmol, POB 2450, Stanford, CA 94305 USA
[19] IIT Hyderabad, Dept Phys, Kandi 502285, Telangana, India
[20] CALTECH, Jet Prop Lab, 4800 Oak Grove Dr, Pasadena, CA 91109 USA
[21] Univ Chicago, Kavli Inst Cosmol Phys, Chicago, IL 60637 USA
[22] Univ Autonoma Madrid, Inst Fis Teor UAM CSIC, E-28049 Madrid, Spain
[23] Univ Michigan, Dept Phys, Ann Arbor, MI 48109 USA
[24] SLAC Natl Accelerator Lab, Menlo Pk, CA 94025 USA
[25] Univ Washington, Dept Astron, Box 351580, Seattle, WA 98195 USA
[26] Natl Opt Astron Observ, Cerro Tololo Inter Amer Observ, Casilla 603, La Serena, Chile
[27] Australian Astron Observ, N Ryde, NSW 2113, Australia
[28] Inst Catalana Rec & Estud Avancats, E-08010 Barcelona, Spain
[29] Univ Sussex, Dept Phys & Astron, Pevensey Bldg, Brighton BN1 9QH, E Sussex, England
[30] CIEMAT, Madrid, Spain
[31] Univ Fed Rio Grande do Sul, Inst Fis, Caixa Postal 15051, BR-91501970 Porto Alegre, RS, Brazil
[32] Univ Fed ABC, Ctr Ciencias Nat & Humanas, Av Estados 5001, BR-09210580 Santo Andre, SP, Brazil
[33] Oak Ridge Natl Lab, Comp Sci & Math Div, Oak Ridge, TN 37831 USA
基金
澳大利亚研究理事会; 欧洲研究理事会; 美国国家科学基金会; 英国科学技术设施理事会;
关键词
galaxies: abundances; galaxies: dwarf; stars: abundances; stars: chemically peculiar; METAL-POOR STARS; RED GIANT BRANCH; CHEMICAL EVOLUTION; SPECTROSCOPIC ANALYSIS; DETAILED ABUNDANCES; SPHEROIDAL GALAXIES; HEAVY-ELEMENTS; 1ST STARS; S-PROCESS; NUCLEOSYNTHESIS;
D O I
10.3847/1538-4357/aa634a
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Chemically peculiar stars in dwarf galaxies provide a window for exploring the birth environment of stars with varying chemical enrichment. We present a chemical abundance analysis of the brightest star in the newly discovered ultra-faint dwarf galaxy candidate Tucana III. Because it is particularly bright for a star in an ultra-faint Milky Way (MW) satellite, we are able to measure the abundance of 28 elements, including 13 neutron-capture species. This star, DES. J235532.66-593114.9 (DES J235532), shows a mild enhancement in neutron-capture elements associated with the r-process and can be classified as an r-I star. DES. J235532 is the first r-I star to be discovered in an ultra-faint satellite, and Tuc. III is the second extremely low-luminosity system found to contain r-process enriched material, after Reticulum. II. Comparison of the abundance pattern of DES. J235532 with r-I and r-II stars found in other dwarf galaxies and in the MW halo suggests a common astrophysical origin for the neutron-capture elements seen in all r-process enhanced stars. We explore both internal and external scenarios for the r-process enrichment of Tuc. III and show that with abundance patterns for additional stars, it should be possible to distinguish between them.
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页数:11
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