How the Rock became Rockules: Dwayne Johnson’s Star Text in Hercules (2014)

2020 ◽  
pp. 650-666
Keyword(s):  
2019 ◽  
Vol 10 (1) ◽  
pp. 52-74
Author(s):  
Smita Banerjee

This essay focuses on a fragment of the Bengali superstar Uttam Kumar’s star text, the dada figure, to analyse the contours of melodramatic enunciations and masculinity that appear in the 1970s’ popular films. This decade is identified with the radical politics associated with the Naxal movement that erupted in varied expressions of rage and anger at institutional and systemic failures. Since Uttam typified a bhadralok masculine subjectivity, his evolution in domestic melodramas especially in male weepies from the period enables me to read the specifics of regional cinema and its response to social and political contexts of the times.


Author(s):  
Elena D’Amelio

Although fascination with the film star dates back as far as Béla Balázs’s The Visible Man (1924), the study of stars and stardom did not become a commonplace of film studies until the 1980s. The discipline that first approached the mechanics of contemporary celebrity was sociology, which produced some important works in the late 1950s and early 1960s. Barthes 1972, Morin 2005 (both cited under Theorizing Stardom), and Alberoni’s The Powerless Elite (1963) were among the first works to address stardom’s cultural and ideological implications from, respectively, semiotic, philosophical, and sociological standpoints. These three books were all published in late 1950s and early 1960s, a time when celebrity culture was increasingly visible. These studies set the stage for an exploration of stardom, culture, and ideology that culminated with the publication of the influential work Dyer 1998 (cited under Theorizing Stardom). The author introduced the idea of the “star text,” a concept that stretched beyond an artist’s performances in films to include fan magazine articles, advertising posters, personal biographies, and rumors about actors, all of which contribute to the experience of modern celebrity. Since then, “stardom” has encompassed numerous issues in academic film studies, including the star as historical entity; the star as discursive formation and cultural commodity; the role of audience and fandom in the construction of the star; and the star as the intersection of cinematic language and technique with larger historical dynamics, such as gender, sexuality, youth, politics, and fashion.


Author(s):  
Dominic McHugh

This chapter on Barbra Streisand’s first three film musicals considers how her star text affects the adaptation of the three Broadway musicals on which they are based. Although Streisand starred in Funny Girl on the stage, the screen version made significant changes to the musical, relating the story as a flashback so that it could be telescoped through her perspective. Most of the other characters’ songs were cut, a ploy that was also used in On a Clear Day You Can See Forever to emphasize Streisand as the star. In both films, as well as in Hello, Dolly!, Streisand was cast opposite men with weak singing voices, empowering her performance musically in each case. A good example of how this works is in the title song of On a Clear Day, where Yves Montand performs the number complete with a simple orchestration and staging, followed by Streisand’s much grander performance. Meanwhile, in Dolly! it was necessary to make changes to the title character in order to draw attention away from the fact that Streisand was much too young for the role; thus she is depicted as a general busybody in ‘Just Leave Everything to Me,’ which replaced ‘I Put My Hand In,’ which focuses on Dolly as a matchmaker.


2021 ◽  
pp. 129-133
Author(s):  
Billie Holiday ◽  
William Dufty
Keyword(s):  

2016 ◽  
Vol 20 (1) ◽  
pp. 255-271 ◽  
Author(s):  
Elizabeth Ellcessor

Celebrity activism, online celebrity, and online activism are all growing areas of research, but have received relatively little integration. This article argues that connected celebrity activism deploys social media to forge a variety of connections, enabling activist values to pervade a celebrity persona, reinforcing perceptions of authenticity and recirculating those values to disparate audiences. In the case of Deaf American actor Marlee Matlin, media reform activism serves as a unifying feature, expressed via technologically-facilitated connections between her acting, activist, and online activities, creating a cohesive star text that is seemingly authentic in respect to both Deaf and celebrity identities without being stereotypical. Such centrality and unification via connected celebrity activism stands in contrast to more traditional celebrity activism, and draws upon the specific dynamics of digital media, online activism, and contemporary celebrity culture.


2016 ◽  
Vol 462 (2) ◽  
pp. 1470-1500 ◽  
Author(s):  
Rebecca Lange ◽  
Amanda J. Moffett ◽  
Simon P. Driver ◽  
Aaron S. G. Robotham ◽  
Claudia del P. Lagos ◽  
...  
Keyword(s):  

2020 ◽  
Vol 494 (1) ◽  
pp. 1366-1374
Author(s):  
Marcin Sawicki ◽  
Liz Arcila-Osejo ◽  
Anneya Golob ◽  
Thibaud Moutard ◽  
Stéphane Arnouts ◽  
...  

ABSTRACT We study the environments of a sample of 61 extremely rare $z\, \sim$1.6 Ultra-Massive Passively Evolving Galaxies (UMPEGs: stellar masses M⋆ >1011.5 M⊙) which – based on clustering analysis presented in Cheema et al. (2020) – appear to be associated with very massive (Mhalo ∼ 1014.1h−1 M⊙) dark matter haloes that are likely to be the progenitors of $z\, \sim$0 massive (Coma- and Virgo-like) galaxy clusters. We find that UMPEGs on average have fewer than one satellite galaxy with mass ratio $M_{\star }^{\text{sat}}$:$M_{\star }^{{\text{UMPEG}}}$ ≥ 1:5 (i.e. $M_{\star }^{\text{sat}}$$\gtrsim 10^{10.8}$ M⊙) within 0.5 Mpc; the large mass gap that we observe between the typical UMPEG and its most massive satellite implies that the $z\, \sim$1.6 UMPEGs assembled through major mergers. Using observed satellite counts with merger time-scales from the literature, we estimate the growth rate due to mergers with mass ratio of ≥1:4 to be ∼13 per cent Gyr−1 (with a $\sim \, 2 \times$ systematic uncertainty). This relatively low growth rate is unlikely to significantly affect the shape of the massive end of the stellar mass function, whose evolution must instead be driven by the quenching of new cohorts of ultra-massive star-forming galaxies. However, this growth rate is high enough that, if sustained to $z\, \sim$0, the typical $z\, \sim$1.6 $M_{\star }^{{\text{UMPEG}}}$ =1011.6 M⊙ UMPEG can grow into a M⋆ ≈1012 M⊙ brightest cluster galaxy (BCG) of a present-day massive galaxy cluster. Our observations favour a scenario in which our UMPEGs are main-branch progenitors of some of the present-day BCGs that have first assembled through major mergers at high redshifts and grown further through (likely minor) merging at later times.


Author(s):  
Monica S. Cyrino

This chapter examines the biblical patriarch Noah as played by Russell Crowe in Darren Aronofsky’s Noah (2014). Starting from the foundation of Richard Dyer’s idea of a “star text” in which actors bring echoes of their old roles to new performances and thereby engage viewers on multiple levels, this chapter frames Crowe’s performance in Noah as what the author terms a “maximal projection.” Crowe brings his role as Maximus Decimus Meridius, the soldier who becomes a gladiator during the reigns of Marcus Aurelius and Commodus, to his later role as Noah. Through the repetition of things such as physical gestures, bodily movements, interactions with characters, and even sometimes dialogue, Crowe performs what the author terms “star-peats.”


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