Silicon and oxygen abundances in planet-host stars
E Brugamyer, SE Dodson-Robinson… - The Astrophysical …, 2011 - iopscience.iop.org
The positive correlation between planet detection rate and host star iron abundance lends
strong support to the core accretion theory of planet formation. However, iron is not the most …
strong support to the core accretion theory of planet formation. However, iron is not the most …
Silicon And Oxygen Abundances In Planet-Host Stars
E Brugamyer, SE Dodson-Robinson, WD Cochran… - 2011 - repositories.lib.utexas.edu
The positive correlation between planet detection rate and host star iron abundance lends
strong support to the core accretion theory of planet formation. However, iron is not the most …
strong support to the core accretion theory of planet formation. However, iron is not the most …
Silicon and Oxygen Abundances in Planet-host Stars
E Brugamyer, SE Dodson-Robinson… - The Astrophysical …, 2011 - ui.adsabs.harvard.edu
The positive correlation between planet detection rate and host star iron abundance lends
strong support to the core accretion theory of planet formation. However, iron is not the most …
strong support to the core accretion theory of planet formation. However, iron is not the most …
SILICON AND OXYGEN ABUNDANCES IN PLANET-HOST STARS
E Brugamyer, SE Dodson-Robinson… - Astrophysical …, 2011 - inis.iaea.org
[en] The positive correlation between planet detection rate and host star iron abundance
lends strong support to the core accretion theory of planet formation. However, iron is not the …
lends strong support to the core accretion theory of planet formation. However, iron is not the …
SILICON AND OXYGEN ABUNDANCES IN PLANET-HOST STARS
E Brugamyer, SE Dodson-Robinson, WD Cochran… - Astrophysical …, 2011 - osti.gov
The positive correlation between planet detection rate and host star iron abundance lends
strong support to the core accretion theory of planet formation. However, iron is not the most …
strong support to the core accretion theory of planet formation. However, iron is not the most …
[引用][C] SILICON AND OXYGEN ABUNDANCES IN PLANET-HOST STARS
E Brugamyer, SE Dodson-Robinson… - The Astrophysical …, 2011 - cir.nii.ac.jp
SILICON AND OXYGEN ABUNDANCES IN PLANET-HOST STARS | CiNii Research CiNii 国立
情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす …
情報学研究所 学術情報ナビゲータ[サイニィ] 詳細へ移動 検索フォームへ移動 論文・データをさがす …
[PDF][PDF] SILICON AND OXYGEN ABUNDANCES IN PLANET-HOST STARS
E Brugamyer, SE Dodson-Robinson, WD Cochran… - Citeseer
The positive correlation between planet detection rate and host star iron abundance lends
strong support to the core accretion theory of planet formation. However, iron is not the most …
strong support to the core accretion theory of planet formation. However, iron is not the most …
Silicon and Oxygen Abundances in Planet-Host Stars
E Brugamyer, SE Dodson-Robinson… - arXiv preprint arXiv …, 2011 - arxiv.org
The positive correlation between planet detection rate and host star iron abundance lends
strong support to the core accretion theory of planet formation. However, iron is not the most …
strong support to the core accretion theory of planet formation. However, iron is not the most …
[引用][C] SILICON AND OXYGEN ABUNDANCES IN PLANET-HOST STARS
E BRUGAMYER… - The Astrophysical …, 2011 - pascal-francis.inist.fr
SILICON AND OXYGEN ABUNDANCES IN PLANET-HOST STARS CNRS Inist Pascal-Francis
CNRS Pascal and Francis Bibliographic Databases Simple search Advanced search Search by …
CNRS Pascal and Francis Bibliographic Databases Simple search Advanced search Search by …
[PDF][PDF] SILICON AND OXYGEN ABUNDANCES IN PLANET-HOST STARS
E Brugamyer, SE Dodson-Robinson, WD Cochran… - researchgate.net
The positive correlation between planet detection rate and host star iron abundance lends
strong support to the core accretion theory of planet formation. However, iron is not the most …
strong support to the core accretion theory of planet formation. However, iron is not the most …