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

Proceedings provides a timely overview of the latest observations of molecular gas and dust in the Milky Way and in other galaxies. It also covers;

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Low-Metallicity Star Formation (Iau S255)

events in low-metallicity environments; dust and gas as seeds for metal-poor star formation; metal-poor initial mass functions, stellar evolution;

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Galaxies In 3D Across The Universe IAU S

of stars, gas and dust in galaxies near and far. This volume demonstrates how detailed measurements of individual objects are complemented by;

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

The link between the structure of the interstellar medium in galaxies and the star formation process is a fast-growing area;

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Formation and Evolution of Galaxy Outskirts (IAU S321)

The borders between galaxies and the almost empty intergalactic medium are ill-defined regions where gas struggles to form stars. The;

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Spectral Energy Distribution Of Galaxies - Sed 2011 (Iau S28

formation, evolution and emission of stellar and accretion-driven sources of photons, the interaction of the photons with the gaseous and dust;

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Galaxy Evolution and Feedback across Different Environments (IAU S359)

such as: How do galaxies acquire their gas and how efficiently is it transformed into stars? How is the supermassive black hole in a galaxy;

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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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Computational Star Formation (Iau S270)

in the fields of interstellar gas dynamics, star formation and galactic dynamics. It includes numerical techniques for modeling physical;

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Galactic Dynamics in the Era of Large Surveys (IAU S353)

that all aspects of galaxy evolution are strongly influenced by the interplay between the dynamics of stars, gas, and dark matter. IAU;

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Proceedings of the International Astronomical Union Symposia and Colloquia

observations, from stars and stellar orbits through nearby black holes and explosive events, to the building blocks and transport of energy in galaxies;

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Proceedings of the International Astronomical Union Symposia and Colloquia

Planetary nebulae, glowing shells of ionized gas, are the spectacular products of the evolution of low- and intermediate-mass stars. For;

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The Physics and Evolution of Active Galactic Nuclei

spectroscopy, star formation, and the cosmological evolution of galaxies and black holes. This new text by Hagai Netzer, a renowned astronomer and;

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

, and jets, which heat and perhaps remove entirely the interstellar medium of the host galaxy, effectively shutting down star formation. These;

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Star Clusters (IAU S351)

Stellar cluster research is in a dynamic state. IAU Symposium 351 (also chosen as MODEST-19, within the 'Modelling and Observing DEnse;

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The Properties of Star-Forming Galaxies at z~2

through IR photometry, we examine the galaxies' star formation properties, dynamical masses and velocity dispersions, spatially resolved;

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The Magellanic System

are rich in gas, they have been actively forming stars throughout their history, and they display a wealth of dynamical features. Poor;

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Molecular Astrophysics

Focusing on the organic inventory of regions of star and planet formation in the interstellar medium of galaxies, this comprehensive;

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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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Galaxy Masses As Constraints of Formation Models

measure the masses of stars, gas and dark matter in galaxies, and explores what these mass determinations tell us about galaxy evolution. A key;

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The Physics of Interstellar Dust

passing through dust and molecular clouds, astrophysicists need to comprehend the formation and structure of dust clouds and how it collapses to;

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The Physics of Interstellar Dust

passing through dust and molecular clouds, astrophysicists need to comprehend the formation and structure of dust clouds and how it collapses to;

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Secular Evolution Of Galaxies

, and the distribution of a galaxy's constituent stars, gas and dust. This internal evolution is key to understanding cosmological models;

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Starburst Galaxies

located towards the centers of host galaxies. Studies of this kind of star formation at high redshift have produced astonishing results;

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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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