2MASS J10364992+1212199 , the SIMBAD biblio

2MASS J10364992+1212199 , the SIMBAD biblio (33 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST07:53:39


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Title First 3 Authors
2009ApJ...698..865K viz 15       D               1 250 50 Halo streams in the seventh Sloan Digital Sky Survey data release. KLEMENT R., RIX H.-W., FLYNN C., et al.
2010A&A...513A..72B 1320   K A D     X C       35 13 70 Three carbon-enhanced metal-poor dwarf stars from the SDSS. Chemical abundances from CO5BOLD 3D hydrodynamical model atmospheres. BEHARA N.T., BONIFACIO P., LUDWIG H.-G., et al.
2011MNRAS.418..284B viz 38           X         1 115 191 The s-process in low-metallicity stars – II. Interpretation of high-resolution spectroscopic observations with asymptotic giant branch models. BISTERZO S., GALLINO R., STRANIERO O., et al.
2012ApJ...744..195C 16       D               1 35 134 Carbon-enhanced metal-poor stars in the inner and outer halo components of the Milky Way. CAROLLO D., BEERS T.C., BOVY J., et al.
2012ApJ...751...14M 53       D     X         2 50 38 Lithium abundances in carbon-enhanced metal-poor stars. MASSERON T., JOHNSON J.A., LUCATELLO S., et al.
2012MNRAS.422..849B 114           X   F     2 97 85 The s-process in low-metallicity stars - III. Individual analysis of CEMP-s and CEMP-s/r with asymptotic giant branch models. BISTERZO S., GALLINO R., STRANIERO O., et al.
2013AJ....145...13A viz 54       D     X         2 151 146 High-resolution spectroscopy of extremely metal-poor stars from SDSS/SEGUE. I. Atmospheric parameters and chemical compositions. AOKI W., BEERS T.C., LEE Y.S., et al.
2012A&A...548A..34A viz 15       D               4 134 38 Elemental abundances and classification of carbon-enhanced metal-poor stars. ALLEN D.M., RYAN S.G., ROSSI S., et al.
2013ApJ...765..156C viz 15       D               1 26 2 The CH(G) index as a new criterion for selecting red giant stars. CHEN Y.Q., ZHAO G., CARRELL K., et al.
2013A&A...552A.107S 84           X         2 9 131 Carbon-enhanced metal-poor stars: the most pristine objects? SPITE M., CAFFAU E., BONIFACIO P., et al.
2013AJ....146..132L 16       D               1 39 128 Carbon-enhanced metal-poor stars in SDSS/SEGUE. I. Carbon abundance estimation and frequency of CEMP stars. LEE Y.S., BEERS T.C., MASSERON T., et al.
2014ApJ...788..180C viz 15       D               1 329 52 Carbon-enhanced metal-poor stars: CEMP-s and CEMP-no subclasses in the halo system of the Milky Way. CAROLLO D., FREEMAN K., BEERS T.C., et al.
2014ApJ...797...21P viz 15       D               1 606 226 Carbon-enhanced metal-poor star frequencies in the galaxy: corrections for the effect of evolutionary status on carbon abundances. PLACCO V.M., FREBEL A., BEERS T.C., et al.
2015AJ....149...39A 16       D               4 24 7 High-resolution spectroscopy of extremely metal-poor stars from SDSS/SEGUE. II. Binary fraction. AOKI W., SUDA T., BEERS T.C., et al.
2015A&A...579A..28B viz 79           X         2 46 146 TOPoS. II. On the bimodality of carbon abundance in CEMP stars. Implications on the early chemical evolution of galaxies. BONIFACIO P., CAFFAU E., SPITE M., et al.
2016A&A...591A.118S viz 16       D               1 31408 141 The PASTEL catalogue: 2016 version. SOUBIRAN C., LE CAMPION J.-F., BROUILLET N., et al.
2016ApJ...833...20Y viz 16       D               1 304 147 Observational constraints on first-star nucleosynthesis. I. Evidence for multiple progenitors of CEMP-no stars. YOON J., BEERS T.C., PLACCO V.M., et al.
2017PASJ...69...24M 16       D               1 37 14 Lithium in CEMP-no stars: A new constraint on the lithium depletion mechanism in the early universe. MATSUNO T., AOKI W., SUDA T., et al.
2017AJ....154...52M viz 929       D     X         24 68 12 High-resolution spectroscopy of extremely metal-poor stars from SDSS/SEGUE. III. Unevolved stars with [Fe/H] <= -3.5. MATSUNO T., AOKI W., BEERS T.C., et al.
2018A&A...618A.133C viz 42           X         1 7 15 Non-standard s-process in massive rotating stars. Yields of 10-150 M☉ models at Z = 10–3. CHOPLIN A., HIRSCHI R., MEYNET G., et al.
2019MNRAS.490.2241A viz 16       D               1 1012 50 The Pristine survey - VI. The first three years of medium-resolution follow-up spectroscopy of Pristine EMP star candidates. AGUADO D.S., YOUAKIM K., GONZALEZ HERNANDEZ J.I., et al.
2019A&A...632A..62C 81             C       2 261 ~ Inferring the velocity of early massive stars from the abundances of extremely metal-poor stars. CHOPLIN A., TOMINAGA N. and ISHIGAKI M.N.
2020A&A...634A..72S 16       D               1 83 ~ An empirical metallicity tracer in CEMP and C-normal stars. SINGH D., HANSEN C.J., BYRGESEN J.S., et al.
2020ApJ...894...34D viz 16       D               1 24035 ~ The metallicity gradient and complex formation history of the outermost halo of the Milky Way. DIETZ S.E., YOON J., BEERS T.C., et al.
2020ApJ...896...28V 41           X         1 2 ~ Coproduction of light and heavy (r-process) elements via fission deposition. VASSH N., MUMPOWER M.R., McLAUGHLIN G.C., et al.
2021A&A...651A..79B viz 17       D               2 57451 21 TOPoS. VI. The metal-weak tail of the metallicity distribution functions of the Milky Way and the Gaia-Sausage-Enceladus structure. BONIFACIO P., MONACO L., SALVADORI S., et al.
2021ApJ...923..183L viz 17       D               1 147 ~ Fuzzy cluster analysis: application to determining metallicities for very metal-poor stars. LI H.
2022ApJS..259...60R viz 17       D               1 139 22 SEGUE-2: Old Milky Way Stars Near and Far. ROCKOSI C.M., SUN LEE Y., MORRISON H.L., et al.
2022ApJ...931..146A viz 17       D               1 423 7 Four-hundred Very Metal-poor Stars Studied with LAMOST and Subaru. I. Survey Design, Follow-up Program, and Binary Frequency. AOKI W., LI H., MATSUNO T., et al.
2023ApJ...943...23S viz 17       D               1 1792 5 The R-Process Alliance: Chemodynamically Tagged Groups. II. An Extended Sample of Halo r-process-enhanced Stars. SHANK D., BEERS T.C., PLACCO V.M., et al.
2023ApJ...947...23Z viz 17       D               1 647 14 Chemodynamically Tagged Groups of CEMP Stars in the Halo of the Milky Way. I. Untangling the Origins of CEMP-s and CEMP-no Stars. ZEPEDA J., BEERS T.C., PLACCO V.M., et al.
2025ApJ...992...36V 65       D     X         2 42 ~ Classifying Metal-poor Stars with Machine Learning Using Nucleosynthesis Calculations. VASSH N., WANG Y., WOLOSHYN R.M., et al.
2026ApJ...997...44R 720       D     X C       14 20 ~ Abundance of Heavy r-process Elements in CEMP-rs Stars: The Role of the i-process. RIYAS A.M., KARINKUZHI D., VAN ECK S., et al.

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