Masculinities, affect and the (re)place(ment) of stardom in Formula One fan leisure practices

Writing from an autoethnographic perspective, this article explores male leisure practices via the mediated relationships fans enter into with stars. More specifically, my own fandom for Formula One driver Jacques Villeneuve is the locus of study, revealing how this affective investment shapes and furnishes my corresponding leisure practices. Notions of gendered 'performativity' come to the fore, with my own displays evoking, enacting and revealing oscillating performances of masculinity. Moreover, there are interesting gendered dynamics that such fan leisure practices flag in terms of the intersection of female/male relationships and the potential 'fantasy' and/or narcissistic readings that a male fan identifying with and performing as another male sport star afford. Finally, my research reveals paradoxes for contemporary masculinities, with fans reliant upon mediation and commodification to facilitate and sustain their performative roles. © 2011 Taylor & Francis

TOI-1431b/MASCARA-5b: a highly irradiated ultrahot Jupiter orbiting one of the hottest and brightest known exoplanet host stars

Stars and planetary system

TOI-257b (HD 19916b): A warm sub-saturn orbiting an evolved F-type star

We report the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The transit signal was detected by TESS and confirmed to be of planetary origin based on radial velocity observations. An analysis of the TESS photometry, the Minerva-Australis, FEROS, and HARPS radial velocities, and the asteroseismic data of the stellar oscillations reveals that TOI-257b has a mass of MP = 0.138 ± 0.023 M J (43.9 ± 7.3, M⊕), a radius of RP = 0.639 ± 0.013 R J (7.16 ± 0.15, R ⊕), bulk density of 0.65+0.12-0.11 (cgs), and period 18.38818 +0.00085 -0.00084 days. TOI-257b orbits a bright (V = 7.612 mag) somewhat evolved late F-type star with M∗ = 1.390 ± 0.046 rm M sun, R∗ = 1.888 ± 0.033 Rsun, Teff = 6075 ± 90 rm K, and vsin i = 11.3 ± 0.5 km s-1. Additionally, we find hints for a second non-transiting sub-Saturn mass planet on a ∼71 day orbit using the radial velocity data. This system joins the ranks of a small number of exoplanet host stars (∼100) that have been characterized with asteroseismology. Warm sub-Saturns are rare in the known sample of exoplanets, and thus the discovery of TOI-257b is important in the context of future work studying the formation and migration history of similar planetary systems

The Spitzer Microlensing Program As A Probe For Globular Cluster Planets: Analysis Of Ogle-2015-BLG-0448

The microlensing event OGLE-2015-BLG-0448 was observed by Spitzer and lay within the tidal radius of the globular cluster NGC 6558. The event had moderate magnification and was intensively observed, hence it had the potential to probe the distribution of planets in globular clusters. We measure the proper motion of NGC 6558 (${{\boldsymbol{\mu }}}_{\mathrm{cl}}(N,E)=(+0.36\pm 0.10,+1.42\pm 0.10)\;{\rm{mas}}\;{{\rm{yr}}}^{-1}$) as well as the source and show that the lens is not a cluster member. Even though this particular event does not probe the distribution of planets in globular clusters, other potential cluster lens events can be verified using our methodology. Additionally, we find that microlens parallax measured using Optical Gravitational Lens Experiment (OGLE) photometry is consistent with the value found based on the light curve displacement between the Earth and Spitzer

Lipid content and composition of three species of Antarctic fish in relation to buoyancy

The lipip content and composition of various tissues from three species of nototheniid fish from McMurdo Sound, Antarctic have been examined in relation to their habitat and buoyancy. The pelagic midwater Dissostichus mawsoni is neutrally buoyant. It is rich in lipid which is located subcutaneously, as adipose tissue associated intimately with white muscle, and as lipid droplets within the cells of various tissues. White muscle, red muscle and liver are particularly lipid-rich, although the liver is not positively buoyant. The amount of lipid stored in the white muscle increases towards the centre of buoyancy of the fish. These deposits are documented at the anatomical, histological and ultrastructural levels. Tissues of Pagothenia borchgrevinki contain less lipid than D. mawsoni, but liver, red muscle and white muscle are still very rich in lipid. This species is cryopelagic, that is it spends most of the time in the water column just beneath the surface ice layer. It is not neutrally buoyant, but has a low weight in seawater. The tissues of the benthic Trematomus bernacchii contain only normal levels of lipid. The lipid class compositions of all three species are dominated by triacylglycerol, particularly when lipid contents are high. Serum lipids are an exception in containing high levels of the transport lipid sterol ester. The reason why Antarctic fish use triacylglycerols for buoyancy rather than was esters (as used by many myctophids) or squalene (as used by some sharks) is unclear

Aspects of gonadal morphology in the South georgian plunderfish Artedidraco mirus (Perciformes: Artedidraconidae)

Research on reproduction in Antarctic fishes has been primarily focused on evaluation of macroscopic features while microscopic studies have been limited to very few species. In particular no data are available on plunderfishes of the family Artedidraconidae. In order to provide a preliminary description of gonads in the South Georgian plunderfish Artedidraco mirus morphological observations on ovary and testis were carried out using both macroscopic and histological approaches. All fishes were collected during the ICEFISH cruise, at South Georgia Island in June 2004. The ovary was a typical hollow structure: from the ovarian wall connective tissue projected into the ovarian cavity forming ovigerous folds where oocytes were located. The testis was of the lobular-type with lobules defined by connective tissue septa within the testicular wall. The presence of specimens showing post-spawning features suggested that the spawning process was being concluded during the sampling period