Thompson, I.B., et al.: Cluster AgeS Experiment: The age and dis- tance of the globular cluster ω Centauri determined from obser- vations of the eclipsing binary OGLEGC 17. AJ 121, 3089-3099 (2001)I. B. Thompson et al. Cluster AgeS Experiment: The age and distance of the globular...
As the diets of children are relatively stable at the ages of 3–4 [50], the dietary assessments conducted at 3 years of age in this study can be considered as a proxy for dietary intakes at 4 years of age, the timepoint at which the gut microbiome of the study participants was ...
In addition, as its existing data ages, the peer in detention will contain relatively older data compared to other peers. Since most searches focus on newer data, this means that the peer's data will typically get searched less frequently, shifting the burden of the search load onto the peer...
3.6 for the recent extension to lower ages. For most elements, we adopt the usual spectroscopic notation, i.e., \({[X]}=\log {X_{\mathrm{star}}} -\log {X_\odot }\) for any abundance quantity X, and \(\log {\epsilon (X)} = \log {N_{{X}}/N_{\mathrm{H}}} + 12.0...
The central parsec around the supermassive black hole (SMBH) Sgr A* contains a large number of stars that constitute the Nuclear Star Cluster (NSC)1, which is one of the densest and most massive stellar systems in the Galaxy. These stars vary in terms of their ages, masses, sizes, and...
The Read chapters are fixed in the same place for all groups so that the morbidity associations can be visually compared easily between groups. There was greater interconnectedness in populations with eczema and asthma compared with controls, in women compared to men, and in older diagnostic ages ...
Rotation periods are now known for stars in an open cluster of intermediate age (NGC 6819; 2.5Gyr old), and for old field stars whose ages have been determined with asteroseismology. The data for the cluster agree with previous ... JL Van Saders,T Ceillier,TS Metcalfe,... - 《Nature》...
Initial stellar masses were inferred from four isochrones covering ages from 3 to 5 Myr and two sets of stellar evolution models. For each isochrone, the present-day mass function of stars was determined for the full sample of main sequence cluster members using an equal number binning scheme....
We found 877 cluster candidates and we derived their ages, initial masses and extinctions by means of a comparison between the observed spectral energy distribution and the predictions from cluster synthesis models for instantaneous star formation and solar metallicity. The lack of [OIII]emission in ...
Currently popular models known as gyrochronology are based on a “law” derived by Skumanich (1972) which is predicated on the ages of stars and of star clusters derived from assumption-laden models of stellar and cluster evolution being accurate. Our Sun is the only star for which an age ...