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in the fields of interstellar gas dynamics, star formation and galactic dynamics. It includes numerical techniques for modeling physical;
Vergelijkbare producten zoals Computational Star Formation (Iau S270)
formation modes from solar system scales to galaxy scales. IAU Symposium 315 aims to build a coherent picture of how star formation is fueled on a;
Vergelijkbare producten zoals From Interstellar Clouds to Star-Forming Galaxies (IAU S315)
dwarf galaxies, because they are metal poor and because of their kinematics and structure, can tell us about how star formation proceeded in the;
Vergelijkbare producten zoals Low-Metallicity Star Formation (Iau S255)
Stars form surrounded by a circumstellar disk which is thought to be the cradle of planets. IAU Symposium 243 highlights the latest;
Vergelijkbare producten zoals Star-Disk Inter In Young Star (IAU S243)
The lives of massive galaxies are affected by many key processes, including gas accretion and star formation, feedback and quenching, black;
Vergelijkbare producten zoals The Intriguing Life of Massive Galaxies (Iau S295)
aspects of theoretical and observational star formation: low-mass star formation; young circumstellar discs; computational methods; triggered star;
Vergelijkbare producten zoals The Labyrinth of Star Formation
In IAU Symposium 282, members of the exoplanet and binary star communities unite for the first time to discuss the state-of-the-art;
Vergelijkbare producten zoals From Interacting Binaries To Exoplanets (Iau S282)
related topics including the initial conditions for star formation, observational tracers of star formation and interstellar conditions, and;
Vergelijkbare producten zoals Molecular Gas, Dust, And Star Formation In Galaxies (Iau S29
, with sections dedicated to: Local Group dwarf galaxies; the interstellar medium and star formation in dwarfs; metallicity, massive stars, and;
Vergelijkbare producten zoals Dwarf Galaxies (IAU S344)
Stellar cluster research is in a dynamic state. IAU Symposium 351 (also chosen as MODEST-19, within the 'Modelling and Observing DEnse;
Vergelijkbare producten zoals Star Clusters (IAU S351)
today. Five major topics are covered, spanning from star- and planet-formation through stellar populations to extragalactic chemistry and dark;
Vergelijkbare producten zoals Laboratory Astrophysics (IAU S350)
graduate students working in areas relating to galaxy formation and evolution, star formation, dust and stellar populations.;
Vergelijkbare producten zoals Galaxies In 3D Across The Universe IAU S
techniques, before looking at the physics of gas giant atmospheres and close-in stars. The topics of planet formation, migration and the dynamical;
Vergelijkbare producten zoals Proceedings of the International Astronomical Union Symposia and Colloquia
fields of research discuss galactic dynamics, the physics of the interstellar medium and star formation, and the fundamental properties and;
Vergelijkbare producten zoals The Magellanic System
of galaxy formation. The topics covered include downsizing and star-formation time scales in massive elliptical galaxies, the connection between the;
Vergelijkbare producten zoals AGN Feedback in Galaxy Formation
IAU Symposium 346. Taking an interdisciplinary approach, it includes reviews on massive star winds and HMXB donors, Be Stars in the X-ray;
Vergelijkbare producten zoals High-mass X-ray Binaries (IAU S346)
irradiance. Combined study of the spots on the Sun and on other stars provides a greater understanding of sunspot formation and behaviour on a long;
Vergelijkbare producten zoals Physics Of Sun And Star Spots (Iau S273)
concentrated dense gas reservoir and its most extreme star-formation environment. The Galactic Centre is therefore our nearest analogue to both an;
Vergelijkbare producten zoals The Multi-Messenger Astrophysics of the Galactic Centre (IAU S322)
, and jets, which heat and perhaps remove entirely the interstellar medium of the host galaxy, effectively shutting down star formation. These;
Vergelijkbare producten zoals Co-evolution of Central Black Holes and Galaxies (IAU S267)
center fuelled to become an AGN? What is the main physical mechanism that quenches star formation? How powerful are the stellar and AGN feedback;
Vergelijkbare producten zoals Galaxy Evolution and Feedback across Different Environments (IAU S359)
eminent scientists in the field, the book reviews the physical processes related to star formation, starting from cosmological down to galactic;
Vergelijkbare producten zoals Star Formation in Galaxy Evolution: Connecting Numerical Models to Reality
eminent scientists in the field, the book reviews the physical processes related to star formation, starting from cosmological down to galactic;
Vergelijkbare producten zoals Star Formation in Galaxy Evolution Connecting Numerical Models to Reality
A major fraction of star formation in the universe occurs in starbursts. These regions of particularly rapid star formation are often;
Vergelijkbare producten zoals Starburst Galaxies
Guiding the reader through all the stages that lead to the formation of a star such as our Sun, this advanced textbook provides students;
Vergelijkbare producten zoals Introduction To Star Formation
habitable exoplanets. IAU Symposium 328 brings together diverse, interdisciplinary reviews and research papers which address the themes of star;
Vergelijkbare producten zoals Living around Active Stars (IAU S328)
unprecedented temporal and spatial resolutions. This volume includes recent results in solar physics research presented at the IAU Symposium 327, the;
Vergelijkbare producten zoals Fine Structure and Dynamics of the Solar Photosphere (IAU S327)
IAU Symposium 310 takes a broad look at the complexity of planetary systems, in terms of the formation and dynamical evolution of planets;
Vergelijkbare producten zoals Complex Planetary Systems (IAU S310)
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