NGC 7790 50 , the SIMBAD biblio

NGC 7790 50 , the SIMBAD biblio (11 results) C.D.S. - SIMBAD4 rel 1.8 - 2024.04.24CEST22:38:27

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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
1958ApJ...128..150S 141 69 Cepheids in galactic clusters. I. CF Cas (sic) in NGC 7790. SANDAGE A.
1984ApJ...286..563P 399 22 Photographic photometry of the open cluster NGC 7790. PEDREROS M., MADORE B.F. and FREEDMAN W.L.
1989MNRAS.240..459R 197 32 CCD photometry of galactic open clusters - I. NGC 7790. ROMEO G., BONIFAZI A., FUSI PECCI F., et al.
2000A&AS..145..365G viz 1123 8 A complete photometric study of the open cluster NGC 7790 containing Cepheid variables. GUPTA A.C., SUBRAMANIAM A., SAGAR R., 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.
2019ApJ...872..137S viz 17       D               1 26099 39 Constraining metallicity-dependent mixing and extra mixing using [C/N] in alpha-rich field giants. SHETRONE M., TAYAR J., JOHNSON J.A., et al.
2019ApJ...879...69T viz 17       D               1 222609 141 The Payne: self-consistent ab initio fitting of stellar spectra. TING Y.-S., CONROY C., RIX H.-W., et al.
2019AJ....158..147H viz 17       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.
2020AJ....160..120J viz 17       D               1 365761 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.
2020ApJ...900....4S viz 17       D               1 121537 14 The age distribution of stars in the Milky Way bulge. SIT T. and NESS M.K.
2020ApJ...903...55P viz 17       D               1 12300 12 Open cluster chemical homogeneity throughout the Milky Way. POOVELIL V.J., ZASOWSKI G., HASSELQUIST S., et al.

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