Elemental Abundance Determination We / the Sun / Bernstein / Mn Co / Cr I Cr II Mn I Co / MOOG / Stellar Parameter Determination We / The star / /
Country
Russia / Australia / /
Event
Product Issues / /
Facility
St. Petersburg State University / Sobolev Astronomical Institute / Pulkovo Astronomical Observatory / McDonald Observatory / Las Campanas Observatory / University of Michigan / National Optical Astronomy Observatory / /
IndustryTerm
search strategies / final self-consistent solution / chemical abundance patterns / chemical evolution / searches employing data products / metal pollution / chemical elements / chemical composition studies / chemical and dynamical conditions / even other nearby planetary systems / chemical standpoint / chemical compositions / chemical composition / spectroscopic solutions / solar sibling search / Daughter products / chemical tagging / chemical analysis / solar chemical composition / gas giant / gas giant planet / metal-poor / gas cloud / /
Organization
Australian Centre for Astrobiology / Association of Universities for Research / National Science Foundation / School of Physics / Association of Universities / Yale / University of Michigan / Sobolev Astronomical Institute / Univ. of Texas / Department of Astronomy / V (mag) / OB association / St. Petersburg State University / /
Person
Gaia / Al I Si / Al V Y Ba / Al V Y Ba Fe Na Al V / Clay Telescope / Ti I Ti II VI / /
T O APPEAR IN THE A STROPHYSICAL J OURNAL Preprint typeset using LATEX style emulateapj v[removed]ELEMENTAL ABUNDANCES OF SOLAR SIBLING CANDIDATES I. R AM´I REZ 1 , A. T. BAJKOVA 2 , V. V. B OBYLEV 2,3 , I. U. ROEDERER