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Feebly-interacting particles: FIPs 2022 Workshop Report
Particle physics today faces the challenge of explaining the mystery of dark matter, the origin of matter over anti-matter in the Universe, the...
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Pulkovo Observatory and the National Observatory Movement: A Historical Overview
The patronage of national governments has played an important role in the history of astronomy, classically in the form of national observatories. In...
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Charged Particle Acceleration
The momentum and energy of a charged particle obey the equations, where the momentum p = γm o v and γ = (1 − v 2∕c 2)−1∕2. The kinetic energy...
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Magnetic Field Generation in Stars
Enormous progress has been made on observing stellar magnetism in stars from the main sequence (particularly thanks to the MiMeS, MAGORI and BOB...
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Large-Scale Structure Formation: From the First Non-linear Objects to Massive Galaxy Clusters
The large-scale structure of the Universe formed from initially small perturbations in the cosmic density field, leading to galaxy clusters with up...
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Structures and Components in Galaxy Clusters: Observations and Models
Clusters of galaxies are the largest gravitationally bounded structures in the Universe dominated by dark matter. We review the observational...
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Gravitational wave astronomy: the current status
In the centenary year of Einstein’s General Theory of Relativity, this paper reviews the current status of gravitational wave astronomy across a...
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Clusters and groups of galaxies
Galaxies are not uniformly distributed in space, but instead show a tendency to gather together in galaxy groups and clusters of galaxies. This...
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Catalogue of Minor Planet Names and Discovery Circumstances Addendum 2012–2014
Title page of Giuseppe Piazzi’s book “On the discovery of the new planet CERES FERDINANDEA, the eighth of those known in our solar system”. The...
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Challenges of Manned Interstellar Travel
The scientific information in Part II discusses the challenges of an interstellar mission based on an extensive literature review. It links these...
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Cosmology Through Its Past
One of the characters in the 1950s British comedy radio series, The Goon Show, once remarked that “Everybody’s got to be somewhere.” The answer to...
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Reconstruction and Prediction of Variations in the Open Solar Magnetic Flux and Interplanetary Conditions
Historic geomagnetic activity observations have been used to reveal centennial variations in the open solar flux and the near-Earth heliospheric...
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Multiple populations in globular clusters
Recent progress in studies of globular clusters has shown that they are not simple stellar populations, but rather are made up of multiple...
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Catalogue of Minor Planet Names and Discovery Circumstances
Discovered 1801 Jan. 1 by G. Piazzi at Palermo. (* MC 3, 604) Named after the Roman goddess of corn and harvests, daughter of Rhea {see planet (577)}...
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Exospheres and Energetic Neutral Atoms of Mars, Venus and Titan
Our understanding of the upper atmosphere of unmagnetized bodies such as Mars, Venus and Titan has improved significantly in this decade. Recent...
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Exospheres and Energetic Neutral Atoms of Mars, Venus and Titan
Our understanding of the upper atmosphere of unmagnetized bodies such as Mars, Venus and Titan has improved significantly in this decade. Recent...
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Habitability: from stars to cells
To determine where to search for life in our solar system or in other extrasolar systems, the concept of habitability has been developed, based on...
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The Big Bang and the First 380,000 Years
Bearing witness to our running mantra that within the macrocosm is a reflection of the microcosm, the LHC will enable physicists not only to study...
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What makes a planet habitable?
This work reviews factors which are important for the evolution of habitable Earth-like planets such as the effects of the host star dependent...
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Extreme Star Formation
Extreme star formation includes star formation in starbursts and regions forming super star clusters.We survey the current problems in our...
