Accurate masses and radii of normal stars: modern results and applications

This paper presents and discusses a critical compilation of accurate, fundamental determinations of stellar masses and radii. We have identified 95 detached binary systems containing 190 stars (94 eclipsing systems, and alpha Centauri) that satisfy our criterion that the mass and radius of both stars be known to 3% or better. To these we add interstellar reddening, effective temperature, metal abundance, rotational velocity and apsidal motion determinations when available, and we compute a number of other physical parameters, notably luminosity and distance. We discuss the use of this information for testing models of stellar evolution. The amount and quality of the data also allow us to analyse the tidal evolution of the systems in considerable depth, testing prescriptions of rotational synchronisation and orbital circularisation in greater detail than possible before. The new data also enable us to derive empirical calibrations of M and R for single (post-) main-sequence stars above 0.6 M(Sun). Simple, polynomial functions of T(eff), log g and [Fe/H] yield M and R with errors of 6% and 3%, respectively. Excellent agreement is found with independent determinations for host stars of transiting extrasolar planets, and good agreement with determinations of M and R from stellar models as constrained by trigonometric parallaxes and spectroscopic values of T(eff) and [Fe/H]. Finally, we list a set of 23 interferometric binaries with masses known to better than 3%, but without fundamental radius determinations (except alpha Aur). We discuss the prospects for improving these and other stellar parameters in the near future.Comment: 56 pages including figures and tables. To appear in The Astronomy and Astrophysics Review. Ascii versions of the tables will appear in the online version of the articl

The Structure of Bidisperse Suspensions at Low Reynolds Numbers

We present a simulation technique for the direct simulation of the motion of spherical particles suspended in fluids at low Reynods numbers. We use this method to simulate bidisperse suspensions at varying size ratios of the suspended spheres and compare to analytic results of Batchelor for the low concentration regime. We find that the pair correlation functions indicate that three body hydrodynamic e#ects are significant even at volume fractions of # = 0.01 and lead to a decrease of the settling velocity of the involved particle species. In order to describe the time evolution of the concentration profiles in a suspension that settles into a condensed sediment layer from an initially well-mixed state, we propose an advection-di#usion model. The functional forms of the required hindered settling and hydrodynamic di#usion terms are chosen to describe not only our simulation results but also match other experimental results and asymptotically known theoretical predictions...

Core Models of Receptor Reactions to Evaluate Basic Pathway Designs Enabling Heterogeneous Commitments to Apoptosis

International audienceIsogenic cells can respond differently to cytotoxic drugs, such as the tumor necrosis factor-related apoptosis inducing ligand (TRAIL), with only a fraction committing to apoptosis. Since non-genetic transient resistance to TRAIL has been shown to dependent on caspase-8 dynamics at the receptor level in vitro, here we investigate the core reactions leading to caspase-8 activation, based on mass-action kinetics models, to evaluate the basic mechanisms giving rise to the observed heterogeneous response. In this work, we fit our models to single-cell trajectories of time-resolved caspase-8 activation measured in clonal cells after treatment with TRAIL. Then, we analyse our results to assess the relevance of each model and evaluate how well it captures the extent of biological heterogeneity observed in vitro. Particularly, we focus on a positive feedback loop on caspase-8, the impacts of initial condition variations and the relevance of the caspase-8 degradation