2MASS J16411827+3620496 , the SIMBAD biblio

2MASS J16411827+3620496 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST08:11:27


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Title First 3 Authors
1954AJ.....59..422B 36 34 Globular clusters. II. The tentative identification of the main sequence of population II from photoelectric observations in M 13. BAUM W.A.
1956AJ.....61..254S 58 42 A photographic color-magnitude array of the globular cluster M13. SAVEDOFF M.P.
1979AJ.....84..774C 442 87 Astrometry in the globular cluster M 13. I. New proper motions and membership probabilities. CUDWORTH K.M. and MONET D.G.
1996AJ....112..545P viz 169 100 Proton capture chains in globular cluster stars. I. Evidence for deep mixing based on sodium and magnesium abundances in M13 giants. PILACHOWSKI C.A., SNEDEN C., KRAFT R.P., et al.
1999PASP..111.1233S viz 245 9 Radial velocities of giant stars in globular clusters. SODERBERG A.M., PILACHOWSKI C.A., BARDEN S.C., et al.
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.
2008AJ....136.2050L viz 15       D               2 674 274 The SEGUE stellar parameter pipeline. II. Validation with galactic globular and open clusters. LEE Y.S., BEERS T.C., SIVARANI T., et al.
2009AJ....137.4282M viz 15       D               1 195 17 Mass outflow and chromospheric activity of red giant stars in globular clusters. II. M13 and M92. MESZAROS Sz., DUPREE A.K. and SZALAI T.
2011AJ....141...89S viz 15       D               2 1053 146 The SEGUE stellar parameter pipeline. IV. Validation with an extended sample of galactic globular and open clusters. SMOLINSKI J.P., LEE Y.S., BEERS T.C., et al.
2011AJ....142..126S viz 15       D               2 576 33 A survey of CN and CH variations in Galactic globular clusters from Sloan Digital Sky Survey spectroscopy. SMOLINSKI J.P., MARTELL S.L., BEERS T.C., et al.
2016AJ....151....7M viz 16       D               2 313 1 Globular and open clusters observed by SDSS/SEGUE: the giant stars. MORRISON H.L., MA Z., CLEM J.L., et al.

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