Streamlining the extensive information from the original, highly acclaimed monograph, this new An Introduction to the Physics of Interstellar Dust provides a concise reference and overview of interstellar dust and the interstellar medium.
Machine Learning for Planetary Science presents planetary scientists with a way to introduce machine learning into the research workflow as increasingly large nonlinear datasets are acquired from planetary exploration missions.
The goal of the Daniel Chalonge School on Astrofundamental Physics is to contribute to a theory of the universe (and particularly of the early universe) up to the marks, and at the scientific height of, the unprecedented accuracy, existent and expected, in the observational data.
Astronomy and Astrophysics Abstracts, which has appeared in semi-annual volumes since 1969, is de- voted to the recording, summarizing and indexing of astronomical publications throughout the world.
Magnetic energy release plays an important role in a wide variety of cosmic objects such as the Sun, stellar coronae, stellar and galactic accretion disks and pulsars.
This book contains review articles of most of the topics addressed at the conf- ence on Simulations of Magnetohydrodynamic turbulence in astrophysics: recent achievements and perspectives which took place from July 2 to 6, 2001 at the Institut Henri Poincar'e in Paris.
Fred Hoyle was one of the most widely acclaimed and colourful scientists of the twentieth century, a down-to-earth Yorkshireman who combined a brilliant scientific mind with a relish for communication and controversy.
This thesis develops the dispersive optical model into a tool that allows for the assessment of the validity of nuclear reaction models, thereby generating unambiguous removal probabilities of nucleons from valence orbits using the electron-induced proton knockout reaction.
Die Sternbilder und die damit verbundenen Mythen helfen, sich am Sternenhimmel zurechtzufinden, und vermitteln die Vielfalt der Bilder der Mythologie und der Sternsagen.
Solar-terrestrial physics deals with phenomena in the region of space between the surface of the Sun and the upper atmosphere of the Earth, a region dominated by matter in a plasma state.
Planetary nebulae are a keystone for the understanding of the evolution of stars, for deep insights into the physical processes prevailing in highly excited dilute nebulae, and for the chemical evolution in galaxies.
This thesis describes the application of a Monte Carlo radiative transfer code to accretion disc winds in two types of systems spanning 9 orders of magnitude in mass and size.
This book provides extended versions of the talks given at the memorial Pomeranchuk-100 Conference, June 5-6, held in the Institute of Theoretical and Experimental Physics, Moscow, Russia and the review of the 2013 Pomeranchuk Prize Winner - Mikhail Shifman.
The Sunday Times BestsellerIn Wonders of the Solar System - the book of the acclaimed BBC TV series - Professor Brian Cox will take us on a journey of discovery where alien worlds from your imagination become places we can see, feel and visit.
This volume presents the state-of-the-art in selected topics across modern nuclear physics, covering fields of central importance to research and illustrating their connection to many different areas of physics.
The purpose and motivation of these lectures can be summarized in the following two questions: * What is the ground state (and its properties) of dense matter?
These are the proceedings of international conference on Numerical As- trophysics 1998 (NAP98), held at National Olympic Memorial Youth Cen- ter, in Tokyo, Japan in the period of March 10 - 13, 1998, and hosted by the National Astronomical Observatory, Japan (NAOJ).
The book presents very recent advances in understanding dark matter, dark energy effects, orbital dynamics of exoplanets around binary stars in non-planar configurations, the orbital dynamics of a moon in the star-planet systems, the orbital dynamics of interstellar interlopers around binary stars, the mechanisms of stellar flares, parameters of white dwarfs atmospheres.