Long-term impact of the coach-athlete relationship on development, health, and wellbeing: stories from a figure skater

Coaches have been shown to detriment athletes’ health, wellbeing and development. Knowledge of this long-term effect and what it means for athletes to live with such stories is under-explored. Using self-narrative, we examine the longlasting impact of the coach-athlete relationship in the stories of a former figure skater, Fanny. Guided by Arthur Frank’s dialogical analysis, we present creative non-fictional stories to show how Fanny made sense of her figure skating experiences, which were framed by a sport investment narrative and a career-wrecking injury that terminated her dream of becoming a professional figure skater. We suggest that if handled as an act of self-care, storytelling can re-configure the dominant coach-athlete relationship and sport investment narrative and help athletes to understand and reconstruct their stories. Finally, we reflect upon the impact of Fanny’s story on her advisers and consider the pedagogical implications of such narrative work in sport coaching and sport education

Control of star formation by supersonic turbulence

Understanding the formation of stars in galaxies is central to much of modern astrophysics. For several decades it has been thought that stellar birth is primarily controlled by the interplay between gravity and magnetostatic support, modulated by ambipolar diffusion. Recently, however, both observational and numerical work has begun to suggest that support by supersonic turbulence rather than magnetic fields controls star formation. In this review we outline a new theory of star formation relying on the control by turbulence. We demonstrate that although supersonic turbulence can provide global support, it nevertheless produces density enhancements that allow local collapse. Inefficient, isolated star formation is a hallmark of turbulent support, while efficient, clustered star formation occurs in its absence. The consequences of this theory are then explored for both local star formation and galactic scale star formation. (ABSTRACT ABBREVIATED)Comment: Invited review for "Reviews of Modern Physics", 87 pages including 28 figures, in pres

A review of elliptical and disc galaxy structure, and modern scaling laws

A century ago, in 1911 and 1913, Plummer and then Reynolds introduced their models to describe the radial distribution of stars in `nebulae'. This article reviews the progress since then, providing both an historical perspective and a contemporary review of the stellar structure of bulges, discs and elliptical galaxies. The quantification of galaxy nuclei, such as central mass deficits and excess nuclear light, plus the structure of dark matter halos and cD galaxy envelopes, are discussed. Issues pertaining to spiral galaxies including dust, bulge-to-disc ratios, bulgeless galaxies, bars and the identification of pseudobulges are also reviewed. An array of modern scaling relations involving sizes, luminosities, surface brightnesses and stellar concentrations are presented, many of which are shown to be curved. These 'redshift zero' relations not only quantify the behavior and nature of galaxies in the Universe today, but are the modern benchmark for evolutionary studies of galaxies, whether based on observations, N-body-simulations or semi-analytical modelling. For example, it is shown that some of the recently discovered compact elliptical galaxies at 1.5 < z < 2.5 may be the bulges of modern disc galaxies.Comment: Condensed version (due to Contract) of an invited review article to appear in "Planets, Stars and Stellar Systems"(www.springer.com/astronomy/book/978-90-481-8818-5). 500+ references incl. many somewhat forgotten, pioneer papers. Original submission to Springer: 07-June-201

The Physics of Star Cluster Formation and Evolution

© 2020 Springer-Verlag. The final publication is available at Springer via https://doi.org/10.1007/s11214-020-00689-4.Star clusters form in dense, hierarchically collapsing gas clouds. Bulk kinetic energy is transformed to turbulence with stars forming from cores fed by filaments. In the most compact regions, stellar feedback is least effective in removing the gas and stars may form very efficiently. These are also the regions where, in high-mass clusters, ejecta from some kind of high-mass stars are effectively captured during the formation phase of some of the low mass stars and effectively channeled into the latter to form multiple populations. Star formation epochs in star clusters are generally set by gas flows that determine the abundance of gas in the cluster. We argue that there is likely only one star formation epoch after which clusters remain essentially clear of gas by cluster winds. Collisional dynamics is important in this phase leading to core collapse, expansion and eventual dispersion of every cluster. We review recent developments in the field with a focus on theoretical work.Peer reviewe

The Effects of Sexed Semen on Embryonic Development to the Blastocyst Stage

Sexed semen (SS) exhibits approximately 80% of the fertilizing ability of conventional semen (CS), and studies have shown that this continues through the 8-cell stage of bovine embryo development. At the time of this study, no information could be found that, when used for IVF and intracytoplasmic sperm injection (ICSI) development, had been carried to the blastocyst stage. In addition, questions have arisen regarding which of the measured sperm parameters are responsible for the difference between the SS and CS and contribute to this decline in fertility. The goals of this project were to evaluate the effects of using sexed sperm as it relates to embryonic development and to determine if any of the differences in sperm parameters affect embryonic development. A preliminary project evaluated SS and CS from 5 bulls for IVF and ICSI. One bull was selected to provide the sperm (both SS and CS) for the trial, and 1752 oocytes were assigned to either IVF or ICSI. The SS and CS were divided among the available oocytes used for IVF and ICSI. Straws were thawed for 30 s at 37°C, and sperm were then evaluated for motility (provided by CASA, SpermVision, MiniTube of America, Verona, WI), morphology, acrosomal integrity (Coomassie and Pope stains), viability, and nuclear decondensation (SYBR Green and HALO). Results for SS v. CS were as follows: motility, 8 v. 26%; viability, 40.6 v. 30%; nuclear decondensation, 40 v. 30%; normal morphology and acrosomal integrity, no differences. Oocytes were obtained from Applied Reproductive Technologies, LLC (Madison, WI). The fertilization rate was consistently lower (Table 1) for both IVF and ICSI when SS were used (Z = 3.65; P = 0.0003), and there was no evidence that this decline in fertilization rate differed for the 2 methods (Z = 0.18; P = 0.86). Nor was there any evidence that the method affected the fertilization rate in general (Z = 0.75; P = 0.45). Thus, the difference was specific for fertilization rate and had no effect on Day 3 cells or Day 7 blastocysts. A higher fertility rate using ICSI would have indicated that a surface membrane factor may have been decreasing the fertility rate with SS because of the elimination of binding factors associated with ICSI. Thus, it may not be the sperm surface membrane that is distorted in the sexing procedure, but likely the integrity of the spermal DNA, as indicated by the increased nuclear decondensation of SS