The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248Variable Stars in the Newly Discovered Milky Way Dwarf Spheroidal Satellite Canes Venatici IOn the Newly Discovered Canes Venatici II dSph GalaxyDiscovery of HE 1523-0901, a Stronglyr-Process-enhanced Metal-poor Star with Detected UraniumThe case for the dual halo of the Milky WayThe formation of the heaviest elementsThe seventh data release of the Sloan Digital Sky SurveyStructure and kinematics of the stellar halos and thick disks of the Milky Way based on calibration stars from Sloan digital sky survey DR7Ther‐Process in Supernova Explosions from the Collapse of O‐Ne‐Mg CoresKinematics of Metal-poor Stars in the Galaxy. III. Formation of the Stellar Halo and Thick Disk as Revealed from a Large Sample of Nonkinematically Selected StarsPulsating variable stars in the Coma Berenices dwarf spheroidal galaxySEGUE: a spectroscopic survey of 240,000 stars with g = 14-20The R-Process Alliance: Chemical Abundances for a Trio of r-process-enhanced Stars—One Strong, One Moderate, and One MildThe R-Process Alliance: Discovery of the First Metal-poor Star with a Combined r- and s-process Element SignatureThe R-process Alliance: First Release from the Southern Search for R-process-enhanced Stars in the Galactic HaloThe r-process Pattern of a Bright, Highly r-process-enhanced Metal-poor Halo Star at [Fe/H] ∼ −2RAVE J203843.2–002333: The First Highly R-process-enhanced Star Identified in the RAVE SurveyBright metal-poor stars from the Hamburg/ESO Survey. II. A chemodynamical analysisObservational constraints on first-star nucleosynthesis. II. Spectroscopy of an ultra metal-poor CEMP-no starHubble Space Telescope near-ultraviolet spectroscopy of bright CEMP-s starsMetal-poor stars observed with the Magellan telescope. III. New extremely and ultra metal-poor stars from SDSS/SEGUE and insights on the formation of ultra metal-poor starsCarbon-enhanced metal-poor star frequencies in the galaxy: corrections for the effect of evolutionary status on carbon abundancesNew detections of arsenic, selenium, and other heavy elements in two metal-poor starsHubble Space Telescope near-ultraviolet spectroscopy of the bright CEMP-no star BD+44{deg}493Hypervelocity star candidates in the SEGUE G and K dwarf sampleSpectroscopy of hot stars in the Galactic haloThe R-Process Alliance: A Comprehensive Abundance Analysis of HD 222925, a Metal-poor Star with an Extreme R-process Enhancement of [Eu/H] = −0.14White paper on nuclear astrophysics and low energy nuclear physics Part 1: Nuclear astrophysicsThe Fourteenth Data Release of the Sloan Digital Sky Survey: First Spectroscopic Data from the Extended Baryon Oscillation Spectroscopic Survey and from the Second Phase of the Apache Point Observatory Galactic Evolution ExperimentSloan Digital Sky Survey IV: Mapping the Milky Way, Nearby Galaxies, and the Distant UniverseThe eleventh and twelfth data releases of the Sloan Digital Sky Survey: final data from SDSS-IIIDiscovery of a dynamical cold point in the heart of the Sagittarius dSph galaxy with observations from the APOGEE projectCharacterizing the SHARDS of disrupted Milky Way satellites with LAMOSTApplication of the SEGUE stellar parameter pipeline to LAMOST stellar spectraEstimation of distances to stars with stellar parameters from LAMOSTFixing the reference frame for PPMXL proper motions using extragalactic sourcesThe first hypervelocity star from the LAMOST surveyAn algorithm for preferential selection of spectroscopic targets in LEGUELAMOST Experiment for Galactic Understanding and Exploration (LEGUE) — The survey's science planProper motions in kapteyn selected area 103: a preliminary orbit for the Virgo stellar stream
P50
Q29307243-BE211389-E17E-484E-8BC8-FBB8D4CB9490Q53952794-48E281E0-20EB-4C61-A531-0FAF544E3228Q53952882-3DB736C4-F51D-44AE-A2E6-43AB9C89A2EDQ54062361-9EB3FE38-D34A-43D3-A69E-C8CC09CA7BA1Q55883629-35F64720-5C19-4CC7-9894-9C308B5BE261Q55885750-0CA4D49B-76FC-4FC7-AEAF-073E83BBE440Q56002067-DAE7ED71-4BB1-494E-AEF8-F1906774481AQ56030907-79519FCF-9722-40CE-BE6A-CC444E774197Q56168465-527212BD-28E7-425F-B1A6-D5E87B48C770Q56168497-49456445-13A8-43AF-9957-30819830028CQ56269165-18F61B31-D42E-4D7F-8627-BC9A2AFA7195Q56432483-7EB79EAB-3B33-4B66-944D-758F8F10A79DQ56958470-2112E189-3781-4497-9295-FBCE543B71CAQ56958485-25CE14D7-FE82-462F-8443-1DABD7AAC783Q56958499-05F6601D-5060-45FE-9A49-7BC9D70A6E82Q56958540-3CB2E134-9DEB-460F-BF95-EAF424BD91B3Q56958552-AD4736C3-B442-43D0-9B8B-28155D631020Q56958559-38C19110-8392-44D9-A852-9DA37CFFA731Q56958565-3D69E962-8DDD-46BE-B8EC-2C0EAC20154CQ56958611-5FA27B09-AC3C-4DF7-869F-8FCFEAA14C1BQ56958623-3D8AD15C-DDEF-4A2F-ADB2-F93E18C8BB4FQ56958658-C2DC2E04-9AD9-4C6F-9D7A-EB131DD1E325Q56958671-267AC2E5-C9F4-4A2E-BE4D-8DA8FFA045DAQ56958680-8DBD5196-9F1D-4BD7-9529-EC3D12974284Q57258085-EFDBA68E-707A-4B78-9288-4839C4869FA3Q57311330-C1ACF4AC-3D07-4D51-8190-29496A6D3BD1Q57404060-270408FF-D9F3-46FC-8BEC-8BC2F5C9B58BQ57426555-046F6BDB-846B-46D9-856A-460415A4EB57Q57442000-8C02A946-DB33-4C03-B561-4C047E8E540FQ57446723-C909017F-7A5E-4AE5-BE22-7B77CC513B5FQ57446741-63B5D10F-C026-4C4F-B1C1-AD24D39C40CAQ57446749-ED3276B7-53B9-42FC-AADB-FA015B24829DQ57448483-2D7C73C7-5775-4B11-B236-E17A66FA9AE3Q57448489-B0ED74CF-ABC9-4768-A912-0EC81AA0E0F3Q57448496-19B1E448-B18B-4C3A-AC0A-762F4037E9FAQ57448498-40B9D9CA-B7F5-4421-A307-D424F12E439FQ57448518-DA3464E0-9C5C-4D1D-AFF1-BD60C48106C9Q57448527-05F2F15D-B390-41BC-A0BE-9DB3FEB1D874Q57448528-9E5D282A-2EBC-4FF0-85F1-31A0F5C8827AQ57448540-A257BC77-E50E-4117-B7FE-07B42FEA4B05
P50
description
astrofysicus
@nl
name
Timothy Beers
@ast
Timothy Beers
@en
Timothy Beers
@es
Timothy Beers
@nl
type
label
Timothy Beers
@ast
Timothy Beers
@en
Timothy Beers
@es
Timothy Beers
@nl
altLabel
Timothy C. Beers
@en
prefLabel
Timothy Beers
@ast
Timothy Beers
@en
Timothy Beers
@es
Timothy Beers
@nl
P106
P21
P31
P569
1957-06-24T00:00:00Z