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Ordbruk och bokstavsskötsel i fysiken

Vi tror vi vet : Recension av R L Numbers & K Kampourakis "Newton's Apple and Other Myths about Science"

Med Virgina Woolf som brygga mellan naturen och kulturen : Recension av P Molander "Allt är vågor. Virginia Woolf och den moderna fysiken"

Den lydige medborgaren : Recension av B R Brown "Planck. Driven by Vision, Broken by War"

Sfärernas musik : Recension av C Rovelli "Seven Brief Lessons on Physics"

Allt vi inte vet : Recension av H Novotny "The Cunning of Uncertainty"

Skilda världar : Recession av M-J Rubenstein "Worlds without End. The Many Lives ofthe Multiverse"

Fyllig guide till våra noblaste forskare

Infallet som krökte tiden och rummet

Probing the vertical abundance structure of the Galactic disc using red clump stars

Measurements of oscillator strengths in V II using charge transfer reactions

News from the quantum zoo

Unversum och dess småttigheter - om samspelet mellan astronomi och elementarpartikelfysik

Har materien charm? Om Psi och andra elementarpartiklar

Hamilton-Jacobi Theory for the Massless Relativistic String

Even quantum pigeons may thrive together

Photometric Characterization of the Earthshine Telescope

Photon Counting in Astronomy: Evaluation of avalanche photodiode detectors

Gaia Early Data Release 3: The Galactic anticentre

Aims. We aim to demonstrate the scientific potential of the Gaia Early Data Release 3 (EDR3) for the study of different aspects of the Milky Way structure and evolution and we provide, at the same time, a description of several practical aspects of the data and examples of their usage. Methods. We used astrometric positions, proper motions, parallaxes, and photometry from EDR3 to select different

Gaia Data Release 2 : Variable stars in the colour-absolute magnitude diagram

Context. The ESA Gaia mission provides a unique time-domain survey for more than 1.6 billion sources with G ≲ 21 mag. Aims. We showcase stellar variability in the Galactic colour-absolute magnitude diagram (CaMD). We focus on pulsating, eruptive, and cataclysmic variables, as well as on stars that exhibit variability that is due to rotation and eclipses. Methods. We describe the locations of var