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Physics Of Sun And Star Spots (Iau S273)

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;

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Fine Structure and Dynamics of the Solar Photosphere (IAU S327)

unprecedented temporal and spatial resolutions. This volume includes recent results in solar physics research presented at the IAU Symposium 327, the;

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Proceedings of the International Astronomical Union Symposia and Colloquia

. The proceedings of IAU Symposium 249 present the latest theoretical and observational advances in the field of exoplanet research, including;

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The Sun as a Star

, Galaxies and The Stars, Roger Tayler presents the first full picture of how studies of the Sun and the solar system help us understand stars;

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The Sun as a Star

. Altogether, this is an invaluable textbook for students studying the Sun, stars, the solar-terrestrial environment and the formation of planetary;

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Living around Active Stars (IAU S328)

The variable activity of stars such as the Sun is mediated through stellar magnetic fields, radiative and energetic particle fluxes;

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The Ages of Stars

efforts to better constrain the ages of individual stars and groups of stars through improved observations and physical models. IAU S258;

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Star-Disk Inter In Young Star (IAU S243)

Stars form surrounded by a circumstellar disk which is thought to be the cradle of planets. IAU Symposium 243 highlights the latest;

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The Multi-Messenger Astrophysics of the Galactic Centre (IAU S322)

concentrated dense gas reservoir and its most extreme star-formation environment. The Galactic Centre is therefore our nearest analogue to both an;

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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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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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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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Reports On Astronomy 2010-2012 (Iau Xxviiia)

presidents and chairpersons of the IAU scientific bodies. Topics covered in this wide-ranging volume include: fundamental astronomy; the Sun 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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Chasing the Sun

A chronicle of humanity's historical, mythological and scientific relationship with the sun draws on various world cultures to explore such;

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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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White Dwarfs as Probes of Fundamental Physics (IAU S357)

of extrasolar planets and fundamental physics. The proceedings of IAU Symposium 357 bring together experts from different branches of science working on;

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Jets At All Scales (Iau S275)

of astrophysical jets on all scales. The proceedings of IAU Symposium 275 present an up-to-date account of our current knowledge of jets and outflows;

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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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Astrophysical Dynamics (IAU S271)

Universe, from stars like our Sun to galaxies. A wide range of temporal and spatial scales are generally present, so instabilities, highly;

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From Interacting Binaries To Exoplanets (Iau S282)

In IAU Symposium 282, members of the exoplanet and binary star communities unite for the first time to discuss the state-of-the-art;

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The Sun as a Guide to Stellar Physics

The Sun as a Guide to Stellar Physics illustrates the significance of the Sun in understanding stars through anexamination of the;

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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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The Dynamic Sun

Our Sun is the nearest star and thus an ideal laboratory to study dynamic processes which are related to solar terrestrial physics;

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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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Seven Spots on the Sun

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Laboratory Astrophysics (IAU S350)

, providing a bridge between observers and modelers. IAU Symposium 350 was organized by the International Astronomical Union's Laboratory Astrophysics;

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