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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)
processes within them. Observations of these nearby dwarf galaxies continue to advance, calibrate and challenge our knowledge of the cosmos. They;
Vergelijkbare producten zoals The Magellanic System
, 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)
Our knowledge of the molecular gas content in galaxies has advanced rapidly in the past decade with systematic surveys from ground-based;
Vergelijkbare producten zoals Molecular Gas, Dust, And Star Formation In Galaxies (Iau S29
IAU Symposium 267 assesses the diverse observational and theoretical attempts to answer the complex question of how quasars physically;
Vergelijkbare producten zoals Co-evolution of Central Black Holes and Galaxies (IAU S267)
Recent observational developments are providing the first truly panchromatic view of galaxies, extending from the radio to TeV gamma rays;
Vergelijkbare producten zoals Spectral Energy Distribution Of Galaxies - Sed 2011 (Iau S28
dust enables the collapse of clouds or how it determines the spectral behaviour of protostars, star forming regions or whole galaxies. This;
Vergelijkbare producten zoals The Physics of Interstellar Dust
dust enables the collapse of clouds or how it determines the spectral behaviour of protostars, star forming regions or whole galaxies. This;
Vergelijkbare producten zoals The Physics of Interstellar Dust
Turbulence is universal and mysterious. It remains one of the major unsolved problems in physics and astrophysics. From star formation to;
Vergelijkbare producten zoals Interstellar Turbulence
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)
physical models can be made to represent the most complex processes. IAU Symposium 270 reviews a wide range of topics relevant to computer modeling;
Vergelijkbare producten zoals Computational Star Formation (Iau S270)
in astronomy during the years 2010-12. These insightful and up-to-date reviews from the IAU Divisions and Commissions have been written by the;
Vergelijkbare producten zoals Reports On Astronomy 2010-2012 (Iau Xxviiia)
articles on the build up of larger galaxies from smaller galaxies and stellar clusters, and discussions of the latest data from large surveys and;
Vergelijkbare producten zoals Star Clusters (IAU S351)
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)
in these discussions spanning from early galaxies to the present day.;
Vergelijkbare producten zoals Galaxy Evolution and Feedback across Different Environments (IAU S359)
IAU Symposium 309 contains contributions on the timely theme of spatially and energetically resolved properties of galaxies. New;
Vergelijkbare producten zoals Galaxies In 3D Across The Universe IAU S
We study the properties of star-forming galaxies at redshift z 2, an era in which a substantial fraction of the stellar mass in the;
Vergelijkbare producten zoals The Properties of Star-Forming Galaxies at z~2
IAU Symposium 356 summarises the most recent results in the field of active galaxies and active galactic nuclei (AGN). These are some;
Vergelijkbare producten zoals Nuclear Activity in Galaxies Across Cosmic Time (IAU S356)
Cosmology at Padova University. From the cold molecular phase in which stars and planetary systems form, to the very hot coronal gas that surrounds;
Vergelijkbare producten zoals Astrophysics of the Interstellar Medium
Cosmology at Padova University. From the cold molecular phase in which stars and planetary systems form, to the very hot coronal gas that surrounds;
Vergelijkbare producten zoals Astrophysics of the Interstellar Medium
In the interstellar medium - the space between the stars in galaxies - new stars are born from material that is replenished by the debris;
Vergelijkbare producten zoals Cambridge Astrophysics
posters presented at the IAU Symposium 323. It should be of interest to researchers and advanced students interested in this field and in related;
Vergelijkbare producten zoals Proceedings of the International Astronomical Union Symposia and Colloquia
Global magnetic fields in planets, in the Sun and other stars, in spiral galaxies and galaxy clusters are believed to be generated and;
Vergelijkbare producten zoals Solar And Astrophysical Dynamos And Magnetic Activity (Iau S
them and other astronomical objects. Recent developments regarding the evolutionary connections between active galaxies and star-forming;
Vergelijkbare producten zoals The Physics and Evolution of Active Galactic Nuclei
; the Sun and heliosphere; planetary sciences; stars; variable stars; interstellar matter; the Galactic system; galaxies and the Universe;
Vergelijkbare producten zoals Reports on Astronomy
(DIBs). The DIBs are a set of hundreds of absorption bands that are seen from the near-ultraviolet to near-infrared wavelengths. Their;
Vergelijkbare producten zoals The Diffuse Interstellar Bands (Iau S297)
interactions, the chemical structure of molecular clouds in the Milky Way and in external galaxies, the chemistry of outflows and their interactions;
Vergelijkbare producten zoals Astrochemistry of Cosmic Phenomena
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