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| Cl* NGC 2099 KRR 10 , the SIMBAD biblio (9 results) | C.D.S. - SIMBAD4 rel 1.8 - 2026.10.19CEST00:10:20 |
Sort references on where and how often the object is cited
trying to find the most relevant references on this object.
More on score
| 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 |
|---|---|---|---|---|---|---|---|---|---|
| 2005ApJ...618L.123K | 1 | 21 | 74 | The initial-final mass relationship: spectroscopy of white dwarfs in NGC 2099 (M37). | KALIRAI J.S., RICHER H.B., REITZEL D., et al. | ||||
| 2005MNRAS.361.1131F | 55 | 117 | The open-cluster initial-final mass relationship and the high-mass tail of the white dwarf distribution. | FERRARIO L., WICKRAMASINGHE D., LIEBERT J., et al. | |||||
| 2008MNRAS.387.1693C | 16 | D | 1 | 75 | 218 | The initial-final mass relationship of white dwarfs revisited: effect on the luminosity function and mass distribution. | CATALAN S., ISERN J., GARCIA-BERRO E., et al. | ||
| 2009ApJ...692.1013S | 16 | D | 1 | 67 | 141 | Semi-empirical white dwarf initial-final mass relationships: a thorough analysis of systematic uncertainties due to stellar evolution models. | SALARIS M., SERENELLI A., WEISS A., et al. | ||
| 2013ApJ...769....7L | 15 | D | 1 | 89 | 15 | The age and stellar parameters of the Procyon binary system. | LIEBERT J., FONTAINE G., YOUNG P.A., et al. | ||
| 2015ApJ...807...90C | 16 | D | 1 | 27 | 16 | Initial-final mass relation for 3 to 4 M☉ progenitors of white dwarfs from the single cluster NGC 2099. | CUMMINGS J.D., KALIRAI J.S., TREMBLAY P.-E., et al. | ||
2016yCat....1.2035M 
|
16 | D | 14271 | ~ | A Catalogue of Spectroscopically Identified White Dwarfs | MCCOOK G.P. and SION E.M. | |||
| 2018ApJ...866...21C | 18 | D | 1 | 97 | 196 | The white dwarf initial-final mass relation for progenitor stars from 0.85 to 7.5 M☉. | CUMMINGS J.D., KALIRAI J.S., TREMBLAY P.-E., et al. | ||
|
2026ApJ...996...69M
|
20 | D | 3 | 310 | ~ | The White Dwarf Initial-Final Mass Relation from Open Clusters in Gaia DR3. | MILLER D.R., CAIAZZO I., HEYL J., et al. |
