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From Interstellar Clouds to Star-Forming Galaxies (IAU S315)

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;

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The Magellanic System

processes within them. Observations of these nearby dwarf galaxies continue to advance, calibrate and challenge our knowledge of the cosmos. They;

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Dwarf Galaxies (IAU S344)

, with sections dedicated to: Local Group dwarf galaxies; the interstellar medium and star formation in dwarfs; metallicity, massive stars, and;

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Molecular Gas, Dust, And Star Formation In Galaxies (Iau S29

Our knowledge of the molecular gas content in galaxies has advanced rapidly in the past decade with systematic surveys from ground-based;

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Co-evolution of Central Black Holes and Galaxies (IAU S267)

IAU Symposium 267 assesses the diverse observational and theoretical attempts to answer the complex question of how quasars physically;

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Spectral Energy Distribution Of Galaxies - Sed 2011 (Iau S28

Recent observational developments are providing the first truly panchromatic view of galaxies, extending from the radio to TeV gamma rays;

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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;

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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;

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Interstellar Turbulence

Turbulence is universal and mysterious. It remains one of the major unsolved problems in physics and astrophysics. From star formation to;

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The Intriguing Life of Massive Galaxies (Iau S295)

The lives of massive galaxies are affected by many key processes, including gas accretion and star formation, feedback and quenching, black;

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Computational Star Formation (Iau S270)

physical models can be made to represent the most complex processes. IAU Symposium 270 reviews a wide range of topics relevant to computer modeling;

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Reports On Astronomy 2010-2012 (Iau Xxviiia)

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;

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Star Clusters (IAU S351)

articles on the build up of larger galaxies from smaller galaxies and stellar clusters, and discussions of the latest data from large surveys and;

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Low-Metallicity Star Formation (Iau S255)

dwarf galaxies, because they are metal poor and because of their kinematics and structure, can tell us about how star formation proceeded in the;

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Galaxy Evolution and Feedback across Different Environments (IAU S359)

in these discussions spanning from early galaxies to the present day.;

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Galaxies In 3D Across The Universe IAU S

IAU Symposium 309 contains contributions on the timely theme of spatially and energetically resolved properties of galaxies. New;

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The Properties of Star-Forming Galaxies at z~2

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;

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Nuclear Activity in Galaxies Across Cosmic Time (IAU S356)

IAU Symposium 356 summarises the most recent results in the field of active galaxies and active galactic nuclei (AGN). These are some;

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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;

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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;

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Cambridge Astrophysics

In the interstellar medium - the space between the stars in galaxies - new stars are born from material that is replenished by the debris;

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Proceedings of the International Astronomical Union Symposia and Colloquia

posters presented at the IAU Symposium 323. It should be of interest to researchers and advanced students interested in this field and in related;

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Solar And Astrophysical Dynamos And Magnetic Activity (Iau S

Global magnetic fields in planets, in the Sun and other stars, in spiral galaxies and galaxy clusters are believed to be generated and;

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The Physics and Evolution of Active Galactic Nuclei

them and other astronomical objects. Recent developments regarding the evolutionary connections between active galaxies and star-forming;

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Reports on Astronomy

; the Sun and heliosphere; planetary sciences; stars; variable stars; interstellar matter; the Galactic system; galaxies and the Universe;

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The Diffuse Interstellar Bands (Iau S297)

(DIBs). The DIBs are a set of hundreds of absorption bands that are seen from the near-ultraviolet to near-infrared wavelengths. Their;

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Astrochemistry of Cosmic Phenomena

interactions, the chemical structure of molecular clouds in the Milky Way and in external galaxies, the chemistry of outflows and their interactions;

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