2MASS J18082002-5104378 , the SIMBAD biblio

2MASS J18082002-5104378 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.13CEST03:05:44

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Bibcode/DOI Score in Title|Abstract|
in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS)
Title First 3 Authors
2016A&A...585L...5M 1085 T K A D   O X C       26 7 11
: The brightest (V = 11.9) ultra metal-poor star.
2018ApJ...857...46I viz 16       D               1 205 88 The initial mass function of the first stars inferred from extremely metal-poor stars. ISHIGAKI M.N., TOMINAGA N., KOBAYASHI C., et al.
2018MNRAS.478.4513B viz 16       D               1 342691 271 The GALAH Survey: second data release. BUDER S., ASPLUND M., DUONG L., et al.
2018ApJ...863..168E 41           X         1 5 1 Revisiting the iron abundance in the hyper iron-poor star HE 1327-2326 with UV COS/HST data. EZZEDDINE R. and FREBEL A.
2018ApJ...867...98S 1402     A D     X C       34 9 33 An ultra metal-poor star near the hydrogen-burning limit. SCHLAUFMAN K.C., THOMPSON I.B. and CASEY A.R.
2019ApJ...871..146F 17       D               1 33 17 Chemical abundance signature of J0023+0307 a second-generation main-sequence star with [Fe/H] < -6. FREBEL A., JI A.P., EZZEDDINE R., et al.
2019MNRAS.484.2166S 436       D S   X   F     9 45 69 Tracing the formation of the Milky Way through ultra metal-poor stars. SESTITO F., LONGEARD N., MARTIN N.F., et al.
2019A&A...624A..44S viz 1990 T K A     X C       46 119 ~ Be and O in the ultra metal-poor dwarf
2MASS J18082002-5104378: the Be-O correlation.
2019MNRAS.487.3797B viz 42           X         1 54 ~ The Pristine survey - V. A bright star sample observed with SOPHIE. BONIFACIO P., CAFFAU E., SESTITO F., et al.
2019A&A...628A.111G viz 84           X         2 9 ~ The 6Li/7Li isotopic ratio in the metal-poor binary CS22876-032. GONZALEZ HERNANDEZ J.I., BONIFACIO P., CAFFAU E., et al.
2020A&A...636A.115D 60       D     X         2 94 38 Reviving old controversies: is the early Galaxy flat or round?. Investigations into the early phases of the Milky Way's formation through stellar kinematics and chemical abundances. DI MATTEO P., SPITE M., HAYWOOD M., et al.
2020A&A...638A.122C viz 43           X         1 88 ~ High-speed stars: Galactic hitchhikers. CAFFAU E., MONACO L., BONIFACIO P., et al.
2020ApJ...904L..22L 128           X         3 7 ~ Investigating the Hubble constant tension: two numbers in the standard cosmological model. LIN W., MACK K.J. and HOU L.
2021A&A...645L...8X viz 17       D               1 9593 36 Local spiral structure based on the Gaia EDR3 parallaxes. XU Y., HOU L.G., BIAN S.B., et al.
2021A&A...646A..70S 131           X C       2 17 ~ Inhomogeneity in the early Galactic chemical enrichment exposed by beryllium abundances in extremely metal-poor stars. SMILJANIC R., ZYCH M.G. and PASQUINI L.
2021MNRAS.503.2539C 88           X         2 29 34 Exploring the Galaxy's halo and very metal-weak thick disc with SkyMapper and Gaia DR2. CORDONI G., DA COSTA G.S., YONG D., et al.
2021ApJ...913...11L viz 17       D               1 1901 19 Targeting bright metal-poor stars in the disk and halo systems of the Galaxy. LIMBERG G., SANTUCCI R.M., ROSSI S., et al.
2021MNRAS.506..150B viz 17       D               1 588596 276 The GALAH+ survey: Third data release. BUDER S., SHARMA S., KOS J., et al.
2021MNRAS.507.3387D 44           X         1 4 ~ MOG cosmology without dark matter and the cosmological constant. DAVARI Z. and RAHVAR S.
2022MNRAS.510.5199C 63           X         1 1 18 Disc fragmentation and oligarchic growth of protostellar systems in low-metallicity gas clouds. CHIAKI G. and YOSHIDA N.
2022ApJ...930...47H 18       D               2 23 6 The GALAH Survey: A New Sample of Extremely Metal-poor Stars Using a Machine-learning Classification Algorithm. HUGHES A.C.N., SPITLER L.R., ZUCKER D.B., et al.
2022MNRAS.517.3993M 3898 T K A D S   X C F     84 5 8 The chemical abundance pattern of the extremely metal-poor thin disc star
and its origins.
2022RNAAS...6..198C 45           X         1 2 ~ [Eu/Ba]: Clock and r-process Indicator. COWLEY C.R. and STENCEL R.E.

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