Astrophysics of Red Supergiants


Book Description

"Astrophysics of Red Supergiants' is the first book of its kind devoted to our current knowledge of red supergiant stars, a key evolutionary phase that is critical to our larger understanding of massive stars. It provides a comprehensive overview of the fundamental physical properties of red supergiants, their evolution, and their extragalactic and cosmological applications. It serves as a reference for researchers from a broad range of fields (including stellar astrophysics, supernovae, and high-redshift galaxies) who are interested in red supergiants as extreme stages of stellar evolution, dust producers, supernova progenitors, extragalactic metallicity indicators, members of massive binaries and mergers, or simply as compelling objects in their own right. The book is accessible to a range of experience levels, from graduate students up to senior researchers."--Source : résumé de l'éditeur.




Astrophysics of Red Supergiants


Book Description

"Astrophysics of Red Supergiants' is the first book of its kind devoted to our current knowledge of red supergiant stars, a key evolutionary phase that is critical to our larger understanding of massive stars. It provides a comprehensive overview of the fundamental physical properties of red supergiants, their evolution, and their extragalactic and cosmological applications. It serves as a reference for researchers from a broad range of fields (including stellar astrophysics, supernovae, and high-redshift galaxies) who are interested in red supergiants as extreme stages of stellar evolution, dust producers, supernova progenitors, extragalactic metallicity indicators, members of massive binaries and mergers, or simply as compelling objects in their own right. The book is accessible to a range of experience levels, from graduate students up to senior researchers."--Source : résumé de l'éditeur.




The Last Stargazers


Book Description

The story of the people who see beyond the stars—an astronomy book for adults still spellbound by the night sky Embark on a captivating cosmic journey with The Last Stargazers. This enthralling book takes you on an awe-inspiring exploration of the night sky, offering a unique perspective on the vast celestial wonders that have fascinated humanity for millennia. Written by astrophysicist Dr. Emily Levesque, The Last Stargazers combines scientific expertise with captivating storytelling, making it the perfect companion for both astronomy enthusiasts and curious minds. Dr. Levesque's passion for the stars shines through as she shares her personal experiences and encounters while working at some of the world's most renowned observatories. Delve into the fascinating world of astronomy as you uncover the secrets of distant galaxies, supernovae, and elusive celestial phenomena. Discover: Inspiring narratives: Dr. Levesque's engaging storytelling transports readers to the front lines of astronomical research, providing a behind-the-scenes glimpse into the life of a modern-day stargazer. Cutting-edge research: Stay up to date with the latest scientific breakthroughs and advancements in the field of astronomy, as Dr. Levesque shares her firsthand experiences and encounters. Accessible explanations: Complex astronomical concepts are made understandable and relatable, allowing readers of all backgrounds to appreciate and comprehend the wonders of the cosmos. Personal perspective: Gain insight into the personal journey of a dedicated scientist as she navigates the challenges and triumphs of studying the stars. Whether you're a seasoned astronomer, a casual stargazer, or simply someone with a curiosity about the universe, The Last Stargazers is an indispensable guide that will ignite your passion for the cosmos and leave you in awe of the wonders that lie beyond. Take a leap into the vast unknown on a celestial odyssey like no other.




The Galaxies of the Local Group


Book Description

The Local Group is a small cluster of galaxies that includes the Milky Way. At least half of all galaxies in the Universe are thought to belong to similar groups. This authoritative volume provides a comprehensive synthesis of what is known about the Local Group. It begins with a summary of each member galaxy, as well as those galaxies previously regarded as possible members. The book examines the mass, stability and evolution of the Local Group as a whole and includes many important previously unpublished results and conclusions. With clarity, Professor van den Bergh provides a masterful summary of all that is known about the galaxies of the Local Group and their evolution, and expertly places this knowledge in the wider context of on-going studies of galaxy formation and evolution, the cosmic distance scale, and the conditions in the early Universe.







An Introduction to the Theory of Stellar Structure and Evolution


Book Description

Using fundamental physics, the theory of stellar structure and evolution can predict how stars are born, how their complex internal structure changes, what nuclear fuel they burn, and their ultimate fate. This textbook is a stimulating introduction for undergraduates in astronomy, physics and applied mathematics, taking a course on the physics of stars. It uniquely emphasises the basic physical principles governing stellar structure and evolution. This second edition contains two new chapters on mass loss from stars and interacting binary stars, and new exercises. Clear and methodical, it explains the processes in simple terms, while maintaining mathematical rigour. Starting from general principles, this textbook leads students step-by-step to a global, comprehensive understanding of the subject. Fifty exercises and full solutions allow students to test their understanding. No prior knowledge of astronomy is required, and only a basic background in physics and mathematics is necessary.




Theory of Stellar Atmospheres


Book Description

The most authoritative synthesis of the quantitative spectroscopic analysis of stellar atmospheres This book provides an in-depth and self-contained treatment of the latest advances achieved in quantitative spectroscopic analyses of the observable outer layers of stars and similar objects. Written by two leading researchers in the field, it presents a comprehensive account of both the physical foundations and numerical methods of such analyses. The book is ideal for astronomers who want to acquire deeper insight into the physical foundations of the theory of stellar atmospheres, or who want to learn about modern computational techniques for treating radiative transfer in non-equilibrium situations. It can also serve as a rigorous yet accessible introduction to the discipline for graduate students. Provides a comprehensive, up-to-date account of the field Covers computational methods as well as the underlying physics Serves as an ideal reference book for researchers and a rigorous yet accessible textbook for graduate students An online illustration package is available to professors at press.princeton.edu




Asymptotic Giant Branch Stars


Book Description

This book deals with stars during a short episode before they undergo a ma jor, and fatal, transition. Soon the star will stop releasing nudear energy, it will become a planetary nebula for abrief but poetic moment, and then it will turn into a white dwarf and slowly fade out of sight. Just before this dramatic change begins the star has reached the highest luminosity and the largest diameter in its existence, and while it is a star detectable in galaxies beyond the Local Group, its structure contains already the inconspicuous white dwarf it will become. It is called an "asymptotic giant branch star" or "AGB star". Over the last 30 odd years AGB stars have become a topic of their own although individual members of this dass had already been studied for cen turies without realizing what they were. In the early evolution, so called "E-AGB"-phase, the stars are a bit bluer than, but otherwise very similar to, what are now called red giant branch stars (RGB stars). It is only in the sec ond half of their anyhow brief existence that AGB stars differ fundamentally from RGB stars.




Handbook of Supernovae


Book Description







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