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Sökning: onr:"swepub:oai:DiVA.org:uu-406910" > The GALAH survey :

  • Lin, JaneAustralian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia;ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia (författare)

The GALAH survey : temporal chemical enrichment of the galactic disc

  • Artikel/kapitelEngelska2020

Förlag, utgivningsår, omfång ...

  • 2019-11-12
  • OXFORD UNIV PRESS,2020
  • printrdacarrier

Nummerbeteckningar

  • LIBRIS-ID:oai:DiVA.org:uu-406910
  • https://urn.kb.se/resolve?urn=urn:nbn:se:uu:diva-406910URI
  • https://doi.org/10.1093/mnras/stz3048DOI

Kompletterande språkuppgifter

  • Språk:engelska
  • Sammanfattning på:engelska

Ingår i deldatabas

Klassifikation

  • Ämneskategori:ref swepub-contenttype
  • Ämneskategori:art swepub-publicationtype

Anmärkningar

  • We present isochrone ages and initial bulk metallicities ([Fe/H](bulk), by accounting for diffusion) of 163 722 stars from the GALAH Data Release 2, mainly composed of main-sequence turn-off stars and subgiants (7000 K > T-eff > 4000 K and log g > 3 dex). The local age-metallicity relationship (AMR) is nearly flat but with significant scatter at all ages; the scatter is even higher when considering the observed surface abundances. After correcting for selection effects, the AMR appears to have intrinsic structures indicative of two star formation events, which we speculate are connected to the thin and thick discs in the solar neighbourhood. We also present abundance ratio trends for 16 elements as a function of age, across different [Fe/H](bulk) bins. In general, we find the trends in terms of [X/Fe] versus age from our far larger sample to be compatible with studies based on small (similar to 100 stars) samples of solar twins, but we now extend them to both sub- and supersolar metallicities. The a-elements show differing behaviour: the hydrostatic alpha-elements O and Mg show a steady decline with time for all metallicities, while the explosive alpha-elements Si, Ca, and Ti are nearly constant during the thin-disc epoch (ages less than or similar to 12 Gyr). The s-process elements Y and Ba show increasing [X/Fe] with time while the r-process element Eu has the opposite trend, thus favouring a primary production from sources with a short time delay such as core-collapse supernovae over long-delay events such as neutron star mergers.

Ämnesord och genrebeteckningar

Biuppslag (personer, institutioner, konferenser, titlar ...)

  • Asplund, MartinAustralian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia;ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia (författare)
  • Ting, Yuan-SenInst Adv Study, Princeton, NJ 08540 USA;Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA;Observ Carnegie Inst Washington, 813 Santa Barbara St, Pasadena, CA 91101 USA (författare)
  • Casagrande, LucaAustralian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia;ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia (författare)
  • Buder, SvenMax Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany (författare)
  • Bland-Hawthorn, JossARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia;Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia (författare)
  • Casey, Andrew R.Monash Univ, Sch Phys & Astron, Clayton, Vic 3800, Australia (författare)
  • De Silva, Gayandhi M.Macquarie Univ, Dept Phys & Astron, Sydney, NSW 2109, Australia (författare)
  • D'Orazi, ValentinaINAF, Osservatorio Astron Padova, Padua, Italy (författare)
  • Freeman, Ken C.Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia;ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia (författare)
  • Kos, JanezUniv Ljubljana, Fac Math & Phys, Jadranska 19, Ljubljana 1000, Slovenia (författare)
  • Lind, KarinUppsala universitet,Institutionen för fysik och astronomi,Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany;Uppsala Univ, Dept Phys & Astron, Observat Astrophys, Box 516, SE-75120 Uppsala, Sweden(Swepub:uu)karli488 (författare)
  • Martell, Sarah L.ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia;Univ New South Wales, Sch Phys, Sydney, NSW 2052, Australia (författare)
  • Sharma, SanjibARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia;Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia (författare)
  • Simpson, Jeffrey D.Univ New South Wales, Sch Phys, Sydney, NSW 2052, Australia (författare)
  • Zwitter, TomazUniv Ljubljana, Fac Math & Phys, Jadranska 19, Ljubljana 1000, Slovenia (författare)
  • Zucker, Daniel B.Macquarie Univ, Dept Phys & Astron, Sydney, NSW 2109, Australia (författare)
  • Minchev, IvanLeibniz Inst Astrophys Potsdam AIP, Sternwarte 16, D-14482 Potsdam, Germany (författare)
  • Cotar, KlemenUniv Ljubljana, Fac Math & Phys, Jadranska 19, Ljubljana 1000, Slovenia (författare)
  • Hayden, MichaelARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia;Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia (författare)
  • Horner, JontiUniv Southern Queensland, Ctr Astrophys, Toowoomba, Qld 4350, Australia (författare)
  • Lewis, Geraint F.Univ Sydney, Sch Phys, Sydney Inst Astron, Sydney, NSW 2006, Australia (författare)
  • Nordlander, ThomasAustralian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia;ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia (författare)
  • Wyse, Rosemary F. G.Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA (författare)
  • Zerjal, MarusaAustralian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia;ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, Australia (författare)
  • Australian Natl Univ, Res Sch Astron & Astrophys, Canberra, ACT 2611, Australia;ARC Ctr Excellence All Sky Astrophys 3 Dimens AST, Sydney, NSW, AustraliaInst Adv Study, Princeton, NJ 08540 USA;Princeton Univ, Dept Astrophys Sci, Princeton, NJ 08544 USA;Observ Carnegie Inst Washington, 813 Santa Barbara St, Pasadena, CA 91101 USA (creator_code:org_t)

Sammanhörande titlar

  • Ingår i:Monthly notices of the Royal Astronomical Society: OXFORD UNIV PRESS491:2, s. 2043-20560035-87111365-2966

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