OXYGEN ABUNDANCES IN LOW- AND HIGH-alpha FIELD HALO STARS AND THE DISCOVERY OF TWO FIELD STARS BORN IN GLOBULAR CLUSTERS


Autoria(s): Ramirez, I.; Melendez, J.; Chaname, J.
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

05/11/2013

05/11/2013

2012

Resumo

Oxygen abundances of 67 dwarf stars in the metallicity range -1.6 < [Fe/H] < -0.4 are derived from a non-LTE analysis of the 777 nm O I triplet lines. These stars have precise atmospheric parameters measured by Nissen and Schuster, who find that they separate into three groups based on their kinematics and alpha-element (Mg, Si, Ca, Ti) abundances: thick disk, high-alpha halo, and low-alpha halo. We find the oxygen abundance trends of thick-disk and high-alpha halo stars very similar. The low-alpha stars show a larger star-to-star scatter in [O/Fe] at a given [Fe/H] and have systematically lower oxygen abundances compared to the other two groups. Thus, we find the behavior of oxygen abundances in these groups of stars similar to that of the a elements. We use previously published oxygen abundance data of disk and very metal-poor halo stars to present an overall view (-2.3 < [Fe/H] < +0.3) of oxygen abundance trends of stars in the solar neighborhood. Two field halo dwarf stars stand out in their O and Na abundances. Both G53-41 and G150-40 have very low oxygen and very high sodium abundances, which are key signatures of the abundance anomalies observed in globular cluster (GC) stars. Therefore, they are likely field halo stars born in GCs. If true, we estimate that at least 3% +/- 2% of the local field metal-poor star population was born in GCs.

NASA through the Sagan Fellowship Program

NASA through the Sagan Fellowship Program

USP (Novos Docentes)

USP (Novos Docentes)

FAPESP [2010/17510-3]

FAPESP

CNPq (Bolsa de Produtividade)

CNPq (Bolsa de Produtividade)

Centro de Astrofisica FONDAP [15010003]

Centro de Astrofisica FONDAP

Centro de Astrofisica y Tecnologias Afines CATA del Proyecto Financiamiento Basal [PFB06]

Centro de Astrofisica y Tecnologias Afines CATA del Proyecto Financiamiento Basal

NASA through Hubble Fellowship [HST-HF-51239.01-A]

NASA through Hubble Fellowship

Space Telescope Science Institute

Space Telescope Science Institute

NASA [NAS5-26555]

NASA

Identificador

ASTROPHYSICAL JOURNAL, BRISTOL, v. 757, n. 2, supl. 1, Part 6, pp. 265-278, OCT 1, 2012

0004-637X

http://www.producao.usp.br/handle/BDPI/41562

10.1088/0004-637X/757/2/164

http://dx.doi.org/10.1088/0004-637X/757/2/164

Idioma(s)

eng

Publicador

IOP PUBLISHING LTD

BRISTOL

Relação

ASTROPHYSICAL JOURNAL

Direitos

closedAccess

Copyright IOP PUBLISHING LTD

Palavras-Chave #GALAXY: DISK #GALAXY: EVOLUTION #GALAXY: FORMATION #GALAXY: HALO #STARS: ABUNDANCES #STARS: POPULATION II #GALACTIC THICK DISK #CENTAURI NGC 5139 #METAL-POOR STARS #SOLAR-TYPE STARS #OMEGA-CENTAURI #MILKY-WAY #MODEL ATMOSPHERES #MAIN-SEQUENCE #GIANT STARS #CHEMICAL ABUNDANCES #ASTRONOMY & ASTROPHYSICS
Tipo

article

original article

publishedVersion