[PDF] Top 20 Studies in stellar structure and evolution

... . Studies o f c la s s ic a l Cepheids (Carson and S to th ers, 1976; S toth ers, 1976a; Vemury and S to th ers, 1978) lead to b etter agreement for in ferred masses and p u lsa tio n a l properties* j between ... See full document

... the evolution of intermediate- to high-mass binary system as their radiative damping serves as the main energy dissipation mechanism in those ...recent studies of intermediate- mass binary systems observed ... See full document

... Earlier studies [6] show that students often do not distinguish between stars and planets and think that the Milky Way is composed by stars that are very close each ...behind evolution of the ...recent ... See full document

... organizational studies should not be ...their evolution and thus are ...Organizational Studies are geared to the definition of new properties in the object of study? Is it possible to think that ... See full document

... and stellar feedback from supernovae, stellar mass-loss, and radiation, enabling a truly “live” response of star formation and the multi-phase ISM to cooling flows; we used a hierarchical super-Lagrangian ... See full document

... for studies of the evolution of supermas- sive black holes is accurate estimates of their ...the evolution of supermassive black hole mass are broad-line AGN, which can be observed to the highest ... See full document

... their studies, K¨ upper et ...Other studies present similar results: the models of disrupted globular clusters performed in Lee et ...the evolution of the cluster can develop a power-law profile with ... See full document

... At this point, as w e prepare to present our results, it would be useful to restate our aims in this work. From the results presented in this chap ter, we hop e to show tha t sm all differences in levels of metallicity, ... See full document

... The evolution of a binary star system by various analytical and numerical approximations of mass transfer rate normalized to the equilibrium rate and its stability conditions are ...star evolution depends ... See full document

... the stellar surface (more precisely one should speak about photosphere, the stellar region from which one can directly receive ...whole stellar structure (but the external parts of the ... See full document

... ABSTRACT Bordetella pertussis causes pertussis, a respiratory disease that is most severe for infants. Vaccination was introduced in the 1950s, and in recent years, a resurgence of disease was observed worldwide, with ... See full document

... the stellar mass versus stellar age relationship, finding a steep trend towards earlier average formation time with increasing stellar mass (downsizing) of ...spectroscopic studies from 0 < ... See full document

... their stellar masses and environmental ...previous studies, suggest an evolutionary link between elliptical and cD ...in stellar mass and size due to ...the stellar masses and sizes of the cDs ... See full document

... in stellar interiors, the third project targeted global properties of shear-driven turbulence and was discussed in Chapter ...In stellar interiors the global shear profile and turbulent length-scales evolve ... See full document

... infrared observations of nearby early–type galaxies, it became apparent that a large, new survey of early–type galaxy properties using imaging detectors was timely. The survey of 327 early–type galaxies described in this ... See full document

... the structure of clusters measured as a function of cluster age hold important clues on the processes of star formation and stellar ...by stellar feedback as well as dynamical interactions between ... See full document

... Recently, new aspects of nuclear dynamics below and around the neutron threshold in nuclei with small and moderate neutron excess has been explored in our studies of low-energy electric and magnetic dipole and ... See full document

... The red dot-dash line and the blue dotted line in Figure 5.17 represent the mean of the two 1.3 and 2.0 cm flux density values between 1978 − 1981 (Newell & Hjellming, 1982) which are not significantly different from ... See full document

... While the discovery occultation of 2013 June 3 provided the general physical parameters of the rings ( width, orientation, orbital radius, optical depth, K) , several questions are still pending, some of which are ... See full document

... Nebulae in an active phase emit energy on their own and show characteristic features in their spectral energy dis- tribution (Lynden-Bell and Pringle, 1974; Adams et al., 1987, 1988). In order to reproduce observational ... See full document