Lithium in a metal-poor external galaxy: ω Centauri

被引:1
|
作者
Bonifacio, P. [1 ,2 ]
Monaco, L. [3 ,4 ]
Sbordone, L. [5 ]
Villanova, S. [3 ]
Pancino, E. [6 ]
机构
[1] Univ Paris Diderot, GEPI, Observ Paris, CNRS, Pl Jules Janssen, F-92190 Meudon, France
[2] Osserv Astron Trieste, Ist Nazl Astrofis, I-34143 Trieste, Italy
[3] Univ Concepcion, Concepcion, Chile
[4] European Southern Observ, Santiago, Chile
[5] Max Planck Inst Astrophys, D-85741 Garching, Germany
[6] Osservatorio Astron Bologna, Ist Nazl Astrofis, I-40127 Bologna, Italy
来源
关键词
Nuclear reactions nucleosynthesis; abundances; stars abundances; Population II; Galaxy globular clusters individual (omega Cen); galaxies abundances; Local Group; cosmology observations; HALO-STARS; ABUNDANCE; SUBGIANT; BRANCH; MODELS;
D O I
10.1017/S1743921310004230
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
omega Centani is it massive stellar system which is currently going through the Galactic Halo Its compact, aspect and spheroidal shape have rot a long time led to it being classified as a Globular Cluster However the fact that its stars cover a wide metallicity range (-0 6 <[Fe/H]< -2.1) points to this object, as an external galaxy. satellite of the Milky Way Lithium among warm metal-poor stilts shows a toughly constant, abundance, the "Spite Plateau" This has been interpreted as evidence lot a primordial origin of the lithium nucleus, at, the time of nucleosynthesis After the physical conditions uncle which nucleosynthesis occurred, have been constrained by the observations of the fluctuations Ions of the Cosmic Microwave Background: we ale facing a "cosmological lithium problem", namely the primordial lithium was a factor of three to four higher than what, observed in the Spite plateau Several avenues may be taken to solve tins conundrum: either relying, on fundamental physics or on stellar physics, however the realin of possibilities may be considerably narrowed by observing stellar populations in different, galaxies, which lime experienced different evolutionary histories Some of the proposed "solutions" may be clearly ruled out, depending on the observation of lithium in the metal-poor populations of external galaxies omega Centauri is the only external galaxy amenable to such an investigation in the era of 8m telescopes We have pushed to its limits FLAMES at, the ESO 8 2m telescope to obtain high resolution spectra of the Li I doublet, in 91 Turn-Off and Sub-Giant stars at V similar to 18 in omega Centauri We present out priliminary results on this data which suggest that the Li content in omega Centauri warm stars is comparable to that observed in Galactic Halo field stars of similar metallicities and temperatures This may effectively title out, a whole class of models which invoke a severe Li depletion through processing of material in an early generation of massive stars
引用
收藏
页码:269 / +
页数:2
相关论文
共 50 条
  • [31] THE CHEMICAL HISTORY OF THE METAL-POOR GALAXY IZW-18
    KUNTH, D
    MATTEUCCI, F
    MARCONI, G
    ASTRONOMY & ASTROPHYSICS, 1995, 297 (03) : 634 - 642
  • [32] The young stellar population of the metal-poor galaxy NGC 6822
    Jones, Olivia C.
    Sharp, Michael J.
    Reiter, Megan
    Hirschauer, Alec S.
    Meixner, M.
    Srinivasan, Sundar
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2019, 490 (01) : 832 - 847
  • [33] LITHIUM ABUNDANCES OF EXTREMELY METAL-POOR TURNOFF STARS
    Aoki, Wako
    Barklem, Paul S.
    Beers, Timothy C.
    Christlieb, Norbert
    Inoue, Susumu
    Perez, E. Garcia
    Norris, John E.
    Carollo, Daniela
    ASTROPHYSICAL JOURNAL, 2009, 698 (02): : 1803 - 1812
  • [34] Lithium isotope ratios in metal-poor halo stars
    Asplund, M
    Lambert, DL
    Nissen, PE
    Primas, F
    Smith, VV
    COSMIC EVOLUTION: ON THE OCCASION OF THE 60TH BIRTHDAYS OF JEAN AUDOUZE AND JAMES W TRURAN, 2001, : 95 - 97
  • [35] Lithium in very metal-poor thick disc stars
    Molaro, P
    Bonifacio, P
    Pasquini, L
    MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1997, 292 (01) : L1 - L4
  • [36] The lithium isotopic ratio in very metal-poor stars
    Lind, K.
    Melendez, J.
    Asplund, M.
    Collet, R.
    Magic, Z.
    ASTRONOMY & ASTROPHYSICS, 2013, 554
  • [37] Lithium isotopic abundances in metal-poor halo stars
    Asplund, Martin
    Lambert, David L.
    Nissen, Poul Erik
    Primas, Francesca
    Smith, Verne V.
    ASTROPHYSICAL JOURNAL, 2006, 644 (01): : 229 - 259
  • [38] Targeting Bright Metal-poor Stars in the Disk and Halo Systems of the Galaxy
    Limberg, Guilherme
    Santucci, Rafael M.
    Rossi, Silvia
    Shank, Derek
    Placco, Vinicius M.
    Beers, Timothy C.
    Schlaufman, Kevin C.
    Casey, Andrew R.
    Perottoni, Helio D.
    Lee, Young Sun
    ASTROPHYSICAL JOURNAL, 2021, 913 (01):
  • [39] The nearby and extremely metal-poor galaxy CGCG 269-049
    Corbin, Michael R.
    Kim, Hwihyun
    Jansen, Rolf A.
    Windhorst, Rogier A.
    Fernandes, Roberto Cid
    ASTROPHYSICAL JOURNAL, 2008, 675 (01): : 194 - 200
  • [40] Dusty Stellar Birth and Death in the Metal-poor Galaxy NGC 6822
    Hirschauer, Alec S.
    Gray, Laurin
    Meixner, Margaret
    Jones, Olivia C.
    Srinivasan, Sundar
    Boyer, Martha L.
    Sargent, B. A.
    ASTROPHYSICAL JOURNAL, 2020, 892 (02):