NGC 6341 9013 , the SIMBAD biblio

NGC 6341 9013 , the SIMBAD biblio (23 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:57:29

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Bibcode/DOI Score in Title|Abstract|
Keywords 		in a table in teXt, Caption, ... Nb occurence Nb objects in ref Citations
(from ADS) 		Title First 3 Authors
1953AJ.....58....4A 28 55 The color-magnitude diagram of the globular cluster M 92. ARP H.C., BAUM W.A. and SANDAGE A.R.
1966ApJ...143..313S 311 177 Three-color photometry of the bright stars in the globular cluster M 92. SANDAGE A. and WALKER M.F.
1976AJ.....81..975C 221 54 Membership and internal motions in the globular cluster M 92. CUDWORTH K.M.
1980AJ.....85..408S 62 61 Calcium abundances in giant stars of the globular clusters M 3, M 13, M 15 and M 92. SUNTZEFF N.B.
1982ApJS...49..207C 76 225 Carbon and nitrogen abundances in giant stars of the metal-poor globular cluster M 92. CARBON D.F., LANGER G.E., BUTLER D., et al.
1983A&AS...53....1B 245 35 Positions, magnitudes, and colors for stars in the globular cluster M 92. BUONANNO R., BUSCEMA G., CORSI C.E., et al.
1992AJ....103.1573R 363 29 New proper motions in the globular clusters M 92. REES R.F.
1992BaltA...1...17Z 68 3 Photoelectric photometry of stars in the areas of globular clusters M 4, M 22, M 71 and M 92. ZDANAVICIUS K.
1996A&A...312...74T viz 470 8 Proper motion study of the globular cluster M 92. TUCHOLKE H.-J., SCHOLZ R.-D. and BROSCHE P.
2000AJ....119.2895P 273 22 A survey for enhanced lithium in 261 globular cluster giants. PILACHOWSKI C.A., SNEDEN C., KRAFT R.P., et al.
2001PASP..113..326B 56 48 Carbon abundances of M92 red giant branch stars. BELLMAN S., BRILEY M.M., SMITH G.H., et al.
2015AJ....149..153M viz 16       D               1 445 139 Exploring anticorrelations and light element variations in northern globular clusters observed by the APOGEE survey. MESZAROS S., MARTELL S.L., SHETRONE M., et al.
2016MNRAS.460.3179W viz 16       D               1 77460 19 Distance and extinction determination for APOGEE stars with Bayesian method. WANG J., SHI J., PAN K., et al.
2018MNRAS.475.1633M viz 16       D               1 383 4 A photometric study of globular clusters observed by the APOGEE survey. MESZAROS S., GARCIA-HERNANDEZ D.A., CASSISI S., et al.
2018AJ....156...18P viz 16       D               1 51824 872 Binary companions of evolved stars in APOGEE DR14: search method and catalog of ∼5000 companions. PRICE-WHELAN A.M., HOGG D.W., RIX H.-W., et al.
2019A&A...622A.191M viz 16       D               1 902 54 Homogeneous analysis of globular clusters from the APOGEE survey with the BACCHUS code. I. The northern clusters. MASSERON T., GARCIA-HERNANDEZ D.A., MESZAROS S., et al.
2019AJ....158...14N viz 16       D               1 1077 40 The relationship between globular cluster mass, metallicity, and light-element abundance variations. NATAF D.M., WYSE R.F.G., SCHIAVON R.P., et al.
2019AJ....158..147H viz 16       D               1 44781 43 Spectrophotometric parallaxes with linear models: accurate distances for luminous red-giant stars. HOGG D.W., EILERS A.-C. and RIX H.-W.
2020MNRAS.492.1641M viz 16       D               1 3434 81 Homogeneous analysis of globular clusters from the APOGEE survey with the BACCHUS code - II. The Southern clusters and overview. MESZAROS S., MASSERON T., GARCIA-HERNANDEZ D.A., et al.
2020AJ....160..120J viz 16       D               1 365763 238 APOGEE data and spectral analysis from SDSS Data Release 16: seven years of observations including first results from APOGEE-South. JONSSON H., HOLTZMAN J.A., ALLENDE PRIETO C., et al.
2022AJ....163..152S viz 17       D               1 583193 11 APOGEE Net: An Expanded Spectral Model of Both Low-mass and High-mass Stars. SPRAGUE D., CULHANE C., KOUNKEL M., et al.
2022ApJS..259...35A viz 17       D               1 611005 320 The Seventeenth Data Release of the Sloan Digital Sky Surveys: Complete Release of MaNGA, MaStar, and APOGEE-2 Data. ABDURRO'UF, ACCETTA K., AERTS C., et al.
2023ApJ...958...45K 17       D               6 52 ~ r-process Abundance Patterns in the Globular Cluster M92. KIRBY E.N., JI A.P. and KOVALEV M.

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