Population synthesis of binary carbon-enhanced metal-poor stars

R.G. Izzard, E. Glebbeek, R.J. Stancliffe, O.R. Pols

Research output: Contribution to journal › Article › Academic › peer-review

Abstract

The carbon-enhanced metal-poor (CEMP) stars constitute approximately one fifth of the metal-poor ([Fe/H]

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title = "Population synthesis of binary carbon-enhanced metal-poor stars",

abstract = "The carbon-enhanced metal-poor (CEMP) stars constitute approximately one fifth of the metal-poor ([Fe/H]",

author = "R.G. Izzard and E. Glebbeek and R.J. Stancliffe and O.R. Pols",

year = "2009",

language = "Undefined/Unknown",

volume = "508",

pages = "1359--1374",

journal = "Astronomy and Astrophysics",

issn = "0004-6361",

publisher = "EDP Sciences",

number = "3",

}

TY - JOUR

T1 - Population synthesis of binary carbon-enhanced metal-poor stars

AU - Izzard, R.G.

AU - Glebbeek, E.

AU - Stancliffe, R.J.

AU - Pols, O.R.

PY - 2009

Y1 - 2009

N2 - The carbon-enhanced metal-poor (CEMP) stars constitute approximately one fifth of the metal-poor ([Fe/H]

AB - The carbon-enhanced metal-poor (CEMP) stars constitute approximately one fifth of the metal-poor ([Fe/H]

M3 - Article

SN - 0004-6361

VL - 508

SP - 1359

EP - 1374

JO - Astronomy and Astrophysics

JF - Astronomy and Astrophysics

IS - 3

ER -