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| NGC 6791 3035 , the SIMBAD biblio (10 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.14CEST23:15:43 |
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 1995AJ....110..693H | 41 | 10 | Optical spectroscopy of the red horizontal branch stars of NGC 6791. | HUFNAGEL B., SMITH G.H. and JANES K.A. | |||||
| 1995AJ....110..823E | 69 | 8 | Blue stragglers in the solar vicinity: newborn or reborn. | EGGEN O.J. | |||||
|
2003PASP..115..413S |
179 | 162 | Homogeneous photometry. III. A star catalog for the open cluster NGC 6791. | STETSON P.B., BRUNTT H. and GRUNDAHL F. | |||||
|
2020AJ....160..120J |
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. | ||
|
2020ApJ...901..109H |
16 | D | 1 | 45439 | 31 | Exploring the stellar age distribution of the Milky Way bulge using APOGEE. | HASSELQUIST S., ZASOWSKI G., FEUILLET D.K., et al. | ||
|
2022AJ....163..152S |
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 |
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. | ||
|
2022ApJ...929...33H |
17 | D | 1 | 114072 | 2 | Quantifying Chemical and Kinematical Properties of Galactic Disks. | HU G. and SHAO Z. | ||
|
2023ApJS..265...50C |
17 | D | 1 | 2291 | ~ | Characterization of Low-mass Companions to Kepler Objects of Interest Observed with APOGEE-N. | CANAS C.I., BENDER C.F., MAHADEVAN S., et al. | ||
|
2023ApJ...950..142H |
17 | D | 1 | 26076 | ~ | Angular Momentum Variation of the Milky Way Thick Disk: The Dependence of Chemical Abundance and Evidence of the Inside-out Formation Scenario. | HU G., SHAO Z. and LI L. |