The Gaia-ESO Survey: evidence of atomic diffusion in M67?
暂无分享,去创建一个
Sergey E. Koposov | E. Grebel | S. Martell | G. Carraro | V. Adibekyan | A. Korn | A. Casey | S. Sousa | U. Heiter | S. Zaggia | M. Costado | S. Randich | A. Lanzafame | S. Blanco-Cuaresma | A. Bragaglia | G. Gilmore | L. Monaco | J. Richer | A. Pasquali | E. Alfaro | G. Sacco | T. Bensby | A. Bayo | E. Franciosini | A. Hourihane | L. Morbidelli | E. Flaccomio | F. Damiani | P. Jofr'e | C. Lardo | L. Magrini | C. Worley | G. Michaud | M. Salaris | R. Smiljanic | A. Drazdauskas | X. Fu | G. Tautvaivsien.e | J. Lewis | C. B. Motta
[1] D. A. García-Hernández,et al. Chemical Abundances of Main-sequence, Turnoff, Subgiant, and Red Giant Stars from APOGEE Spectra. I. Signatures of Diffusion in the Open Cluster M67 , 2018, 1803.04461.
[2] S. Randich,et al. The Gaia-ESO Survey: open clusters in Gaia-DR1 , 2017, Astronomy & Astrophysics.
[3] D. A. García-Hernández,et al. University of Birmingham The Fourteenth Data Release of the Sloan Digital Sky Survey: , 2017 .
[4] T. Nordlander,et al. Non-LTE aluminium abundances in late-type stars , 2017, 1708.01949.
[5] P. Cargile,et al. The Influence of Atomic Diffusion on Stellar Ages and Chemical Tagging , 2017, 1704.03465.
[6] H. Rix,et al. Galactic Doppelgängers: The Chemical Similarity Among Field Stars and Among Stars with a Common Birth Origin , 2017, 1701.07829.
[7] Ulrich Bastian,et al. Hot Stuff for One Year (HSOY) - A 583 million star proper motion catalogue derived from Gaia DR1 and PPMXL , 2017, 1701.02629.
[8] E. Grebel,et al. Observing the products of stellar evolution in the old open cluster M67 with APOGEE , 2017, 1701.00979.
[9] C. Prieto,et al. NLTE ANALYSIS OF HIGH-RESOLUTION H-BAND SPECTRA. I. NEUTRAL SILICON , 2016, 1610.05888.
[10] C. Prieto,et al. NLTE ANALYSIS OF HIGH-RESOLUTION H-BAND SPECTRA. II. NEUTRAL MAGNESIUM , 2016, 1610.05893.
[11] R. Saglia,et al. Search for giant planets in M67 - III. Excess of hot Jupiters in dense open clusters , 2016, 1606.05247.
[12] A. Bragaglia,et al. TheGaia-ESO Survey: Probes of the inner disk abundance gradient , 2016, Astronomy & Astrophysics.
[13] Andrew R Casey,et al. SICK: THE SPECTROSCOPIC INFERENCE CRANK , 2016, 1603.03043.
[14] F. Grundahl,et al. Atomic diffusion and mixing in old stars VI: The lithium content of M30 , 2016, 1603.01565.
[15] Sergey E. Koposov,et al. The Gaia-ESO Survey: Sodium and aluminium abundances in giants and dwarfs. Implications for stellar and Galactic chemical evolution , 2016, 1602.03289.
[16] Nicholas Troup,et al. ASPCAP: THE APOGEE STELLAR PARAMETER AND CHEMICAL ABUNDANCES PIPELINE , 2015, 1510.07635.
[17] J. Richer,et al. Atomic Diffusion in Stars , 2015 .
[18] D. Latham,et al. STELLAR RADIAL VELOCITIES IN THE OLD OPEN CLUSTER M67 (NGC 2682). I. MEMBERSHIPS, BINARIES, AND KINEMATICS , 2015, 1507.01949.
[19] G. Carraro,et al. Testing the chemical tagging technique with open clusters , 2015, 1503.02082.
[20] Annie C. Robin,et al. ABUNDANCES, STELLAR PARAMETERS, AND SPECTRA FROM THE SDSS-III/APOGEE SURVEY , 2015, 1501.04110.
[21] R. S. Ram,et al. SEARCHING FOR CHEMICAL SIGNATURES OF MULTIPLE STELLAR POPULATIONS IN THE OLD, MASSIVE OPEN CLUSTER NGC 6791 , 2014, 1409.8283.
[22] L. Pasquini,et al. The Gaia-ESO Survey: the analysis of high-resolution UVES spectra of FGK-type stars , 2014, 1409.0568.
[23] G. Carraro,et al. Updated properties of the old open cluster Melotte 66: Searching for multiple stellar populations , 2014, 1404.6748.
[24] C. Babusiaux,et al. The Gaia-ESO Survey: processing FLAMES-UVES spectra , 2014 .
[25] L. Pasquini,et al. Three planetary companions around M 67 stars , 2014, 1401.4905.
[26] A. Korn,et al. Abundances and possible diffusion of elements in M 67 stars , 2013, 1310.6297.
[27] N. V. Kharchenko,et al. Global survey of star clusters in the Milky Way II. The catalogue of basic parameters , 2013, 1308.5822.
[28] F. Grundahl,et al. Atomic diffusion and mixing in old stars - IV. Weak abundance trends in the globular cluster NGC 6752 , 2013, 1305.1774.
[29] J. Koppenhoefer,et al. Search for giant planets in M 67. IV. Survey results , 2017, 1703.04296.
[30] S. Lucatello,et al. Searching for multiple stellar populations in the massive, old open cluster Berkeley 39 , 2012, 1211.1142.
[31] L. Girardi,et al. parsec: stellar tracks and isochrones with the PAdova and TRieste Stellar Evolution Code , 2012, 1208.4498.
[32] M. Asplund,et al. Non-LTE line formation of Fe in late-type stars - II. 1D spectroscopic stellar parameters , 2012, 1207.2454.
[33] L. Pasquini,et al. Search for giant planets in M 67 - I. Overview , 2012, 1206.5820.
[34] Sergio Ortolani,et al. The Gaia-ESO Public Spectroscopic Survey , 2012 .
[35] Angela Bragaglia,et al. Multiple populations in globular clusters , 2012, 1201.6526.
[36] A. Weiss,et al. The age of the Milky Way halo stars from the Sloan Digital Sky Survey , 2011, 1105.2022.
[37] M. Asplund,et al. Non-LTE calculations for neutral Na in late-type stars using improved atomic data , 2011, 1102.2160.
[38] A. Korn,et al. M67-1194, an unusually Sun-like solar twin in M67 , 2010, 1009.4579.
[39] J. Anderson,et al. The end of the white dwarf cooling sequence in M 67 , 2010, 1001.3827.
[40] Garching,et al. Intrinsic iron spread and a new metallicity scale for globular clusters , 2009, 0910.0675.
[41] Michael F. Skrutskie,et al. The Apache Point Observatory Galactic Evolution Experiment (APOGEE) in Sloan Digital Sky Survey III (SDSS-III) , 2009, Proceedings of the International Astronomical Union.
[42] A. Dotter,et al. DEEP 2MASS PHOTOMETRY OF M67 AND CALIBRATION OF THE MAIN-SEQUENCE J − KS COLOR DIFFERENCE AS AN AGE INDICATOR , 2009, 0904.2907.
[43] L. Pasquini,et al. Abundances of four open clusters from solar stars , 2008, 0806.2280.
[44] E. Grebel,et al. Comparing CN and CH line strengths in a homogeneous spectroscopic sample of 8 Galactic globular clusters , 2008, 0805.1067.
[45] J. Anderson,et al. Ground-based CCD astrometry with wide-field imagers - II. A star catalog for M 67: WFI@2.2 m MPG/ESO astrometry, FLAMES@VLT radial velocities , 2008, 0803.0004.
[46] Denmark,et al. Atomic Diffusion and Mixing in Old Stars. I. Very Large Telescope FLAMES-UVES Observations of Stars in NGC 6397 , 2007, 0709.0639.
[47] M. Skrutskie,et al. The Two Micron All Sky Survey (2MASS) , 2006 .
[48] L. Pasquini,et al. Element abundances of unevolved stars in the open cluster M 67 , 2006, astro-ph/0601239.
[49] B. Carney,et al. Elemental Abundance Ratios in Stars of the Outer Galactic Disk. I. Open Clusters , 2005, astro-ph/0504193.
[50] R. Gratton,et al. Abundance Variations within Globular Clusters , 2004 .
[51] J. Richer,et al. Models for Solar Abundance Stars with Gravitational Settling and Radiative Accelerations: Application to M67 and NGC 188 , 2004, astro-ph/0402544.
[52] C. Lada,et al. Embedded Clusters in Molecular Clouds , 2003, astro-ph/0301540.
[53] K. Freeman,et al. The New Galaxy: Signatures of Its Formation , 2002, astro-ph/0208106.
[54] J. Richer,et al. Models of Metal-poor Stars with Gravitational Settling and Radiative Accelerations. II. The Age of the Oldest Stars , 2001, astro-ph/0112113.
[55] J. Richer,et al. Iron Convection Zones in B, A, and F Stars , 2001 .
[56] M. Shetrone,et al. Spectroscopy of Blue Stragglers and Turnoff Stars in M67 (NGC 2682) , 2000, astro-ph/0006399.
[57] F. Rogers,et al. Consistent Solar Evolution Model Including Diffusion and Radiative Acceleration Effects , 1998 .
[58] Molefe Mokoene,et al. The Messenger , 1995, Outrageous Fortune.
[59] K. Swamy. Profiles of strong lines in K- dwarfs , 1966 .