Gender trouble in social psychology: How can Butler's work inform experimental social psychologists' conceptualization of gender?

T Morgenroth, MK Ryan - Frontiers in Psychology, 2018 - frontiersin.org
A quarter of a century ago, philosopher Judith called upon society to create “gender trouble”
by disrupting the binary view of sex, gender, and sexuality. She argued that gender, rather …

Accretion disks in luminous young stellar objects

MT Beltrán, WJ de Wit - The Astronomy and Astrophysics Review, 2016 - Springer
An observational review is provided of the properties of accretion disks around young stars.
It concerns the primordial disks of intermediate-and high-mass young stellar objects in …

The dynamics and outcome of star formation with jets, radiation, winds, and supernovae in concert

MY Grudić, D Guszejnov, SSR Offner… - Monthly Notices of …, 2022 - academic.oup.com
We analyse the first giant molecular cloud (GMC) simulation to follow the formation of
individual stars and their feedback from jets, radiation, winds, and supernovae, using the …

Massive star formation

JC Tan, MT Beltrán, P Caselli, F Fontani… - … and Planets VI, 2014 - books.google.com
The enormous radiative and mechanical luminosities of massive stars impact a vast range of
scales and processes, from the reionization of the universe, to the evolution of galaxies, to …

Effects of the environment and feedback physics on the initial mass function of stars in the STARFORGE simulations

D Guszejnov, MY Grudić, SSR Offner… - Monthly Notices of …, 2022 - academic.oup.com
One of the key mysteries of star formation is the origin of the stellar initial mass function
(IMF). The IMF is observed to be nearly universal in the Milky Way and its satellites, and …

A spectroscopic survey on the multiplicity of high-mass stars

R Chini, VH Hoffmeister, A Nasseri… - Monthly Notices of …, 2012 - academic.oup.com
The formation of stars above about 20 M⊙ and their apparently high multiplicity remain
heavily debated subjects in astrophysics. We have performed a vast high-resolution radial …

Formation of massive primordial stars: intermittent UV feedback with episodic mass accretion

T Hosokawa, S Hirano, R Kuiper… - The Astrophysical …, 2016 - iopscience.iop.org
We present coupled stellar evolution (SE) and 3D radiation-hydrodynamic (RHD)
simulations of the evolution of primordial protostars, their immediate environment, and the …

Protostellar feedback halts the growth of the first stars in the Universe

T Hosokawa, K Omukai, N Yoshida, HW Yorke - Science, 2011 - science.org
The first stars fundamentally transformed the early universe by emitting the first light and by
producing the first heavy elements. These effects were predetermined by the mass …

The red MSX source survey: The massive young stellar population of our galaxy

SL Lumsden, MG Hoare, JS Urquhart… - The Astrophysical …, 2013 - iopscience.iop.org
We present the Red MSX Source survey, the largest statistically selected catalog of young
massive protostars and H ii regions to date. We outline the construction of the catalog using …

The formation of massive molecular filaments and massive stars triggered by a magnetohydrodynamic shock wave

T Inoue, P Hennebelle, Y Fukui… - Publications of the …, 2018 - academic.oup.com
Recent observations suggest an that intensive molecular cloud collision can trigger massive
star/cluster formation. The most important physical process caused by the collision is a …