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Stars are mostly found in binary and multiple systems, with at least 50% of all solar-like stars having companions; this fraction approaches 100% for the most massive stars. A large proportion of these systems interact and alter the structure and evolution of their components, leading to exotic objects such as Algol variables, blue stragglers and other chemically peculiar stars, but also to phenomena such as non-spherical planetary nebulae, supernovae and gamma-ray bursts. While it is understood that binaries play a critical role in the Initial Mass Function, the interactions among binary systems significantly affect the dynamical evolution of stellar clusters and galaxies. This interdisciplinary volume presents results from state-of-the-art models and observations aimed at studying the impact of binaries on stellar evolution in resolved and unresolved populations. Serving as a bridge between observational and theoretical astronomy, it is a comprehensive review for researchers and advanced students of astrophysics.
Stars --- Double stars. --- Evolution.
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Stars are mostly found in binary and multiple systems, with at least 50% of all solar-like stars having companions; this fraction approaches 100% for the most massive stars. A large proportion of these systems interact and alter the structure and evolution of their components, leading to exotic objects such as Algol variables, blue stragglers and other chemically peculiar stars, but also to phenomena such as non-spherical planetary nebulae, supernovae and gamma-ray bursts. While it is understood that binaries play a critical role in the Initial Mass Function, the interactions among binary systems significantly affect the dynamical evolution of stellar clusters and galaxies. This interdisciplinary volume presents results from state-of-the-art models and observations aimed at studying the impact of binaries on stellar evolution in resolved and unresolved populations. Serving as a bridge between observational and theoretical astronomy, it is a comprehensive review for researchers and advanced students of astrophysics.
Stars --- Double stars. --- Evolution.
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Extragalactic Novae: A historical perspective takes the reader on a journey chronicling the study of a class of eruptive variable stars known as "Novae Stella", Latin for "New Stars". These mysterious transient objects, now referred to simply as novae, have been recognized since antiquity, suddenly appearing in the night sky before slowly fading back into obscurity. The book begins with a brief introduction to the early observations, including an overview of the role that novae played in the birth of extragalactic astronomy, and concludes with a discussion of how nova observations over the past century have contributed to our knowledge of close binary star populations in nearby galaxies. Along the way, the history of our understanding of the nova phenomena, in the Milky Way and beyond, is unveiled. In particular, the author describes how the enigmatic nova eruptions were finally realized to be the result of thermonuclear runaways on the surfaces of accreting white dwarf stars, how a controversial correlation between a nova's peak luminosity and its rate of decline (the MMRD relation) has been used in extragalactic distance determinations, and how recent observations have bolstered the case that novae may form a significant channel for the production of Type Ia supernovae. These topics, and more, are recounted by an observer who has spent the past 35 years studying these fascinating objects.
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Modern telescopes of even modest aperture can show thousands of double stars. Many are faint and unremarkable but hundreds are worth searching out. Veteran double-star observer Bob Argyle and his co-authors take a close-up look at their selection of 175 of the night sky's most interesting double and multiple stars. The history of each system is laid out from the original discovery to what we know at the present time about the stars. Wide-field finder charts are presented for each system along with plots of the apparent orbits and predicted future positions for the orbital systems. Recent measurements of each system are included which will help you to decide whether they can be seen in your telescope, as well as giving advice on the aperture needed. Double star observers of all levels of experience will treasure the level of detail in this guide to these jewels of the night sky.
Double stars --- Astronomy --- Amateur astronomy.
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Was er ooit een begin of is het heelal er altijd geweest? Kunnen we terugreizen in de tijd? Is er buitenaards leven? Stephen Hawking (1942-2018) was een Brits kosmoloog, natuur- en wiskundige, die geniale theorieën uitwerkte over zwarte gaten en het raadsel van de oerknal. Hij kreeg daarbij extra respect, omdat hij door de ziekte ALS verlamd was en via een spraakcomputer communiceerde. In dit boekje legt Rüdiger Vaas Hawkings fascinerende ideeën op toegankelijke wijze en met veel humor uit. Komische illustraties helpen om de geniale gedachten van de onderzoeker te begrijpen en maken dit boek tot een opwindende reis door Hawkings universum!
Didactics of physics --- Stars --- zwaartekracht --- heelal
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Gas-Phase Chemistry in Space: From elementary particles to complex organic molecules is written by a collection of experts in the field of astrochemistry. The book introduces essential concepts that govern the formation, excitation and destruction of molecules at a postgraduate and research level. A broad range of topics are covered; from early universe chemistry and stellar nucleosynthesis, to the study of bimolecular reaction kinetics. Detailed description of the gas-phase process is provided and recent examples of the interplay between observational and laboratory astrophysics are examined. Using more than 100 figures, as well as examples, this work reveals, in detail, both theoretical and experimental perspectives that can be implemented in future discoveries.
Cosmochemistry. --- Astrophysics. --- Galaxies & stars. --- SCIENCE / Astronomy.
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In CONSTELLATIONS, award-winning astronomy writer Govert Schilling takes us on an unprecedented visual tour of all 88 constellations in our night sky.Much more than just a stargazer's guide, CONSTELLATIONS is complete history of astronomy as told by Schilling through the lens of each constellation. The book is organized alphabetically by constellation. Profiles of each constellation include basic information such as size, visibility, and number of stars, as well as information on the discovery and naming of the constellation and associated lore.Beyond details about the constellation itself is information about every astronomical event that took place or discovery made in the vicinity of the constellation. In the constellation of Cygnus (the Swan) we encounter the location of the first confirmed black hole. A stop at Gemini (the Twins) is a chance to say hello to the dwarf planet Pluto, and in Orion (the hunter) we find the location of the first identified gamma-ray burst.Stunning star maps throughout the book by acclaimed star mapmaker Wil Tirion show us the exact location of every constellation, the details of its structure, as well as its surrounding astronomical neighbors.
Constellations. --- Astronomy --- Stars. --- Constellations --- Étoiles --- Astronomie.
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Modern telescopes of even modest aperture can show thousands of double stars. Many are faint and unremarkable but hundreds are worth searching out. Veteran double-star observer Bob Argyle and his co-authors take a close-up look at their selection of 175 of the night sky's most interesting double and multiple stars. The history of each system is laid out from the original discovery to what we know at the present time about the stars. Wide-field finder charts are presented for each system along with plots of the apparent orbits and predicted future positions for the orbital systems. Recent measurements of each system are included which will help you to decide whether they can be seen in your telescope, as well as giving advice on the aperture needed. Double star observers of all levels of experience will treasure the level of detail in this guide to these jewels of the night sky.
Double stars --- Double stars --- Astronomy --- Amateur astronomy. --- Étoiles doubles. --- Étoiles doubles. --- Astronomie.
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Astronomers study the oldest observable stars in the universe in much the same way archaeologists study ancient artifacts on Earth. Anna Frebel takes readers into the far-flung depths of space and time to provide a gripping firsthand account of the cutting-edge science of stellar archaeology. Weaving the latest findings in astronomy with her own compelling insights as one of the world's leading researchers in the field, she explains how sections of the night sky are "excavated" in the hunt for these extremely rare, 13-billion-year-old relic stars and how this astonishing quest is revealing tantalizing new details about the origins and evolution of the cosmos. Along the way, Frebel recounts her own stories of discovery, offering an insider's perspective on this exciting frontier of science.
Early stars. --- Stars --- Stars --- Galaxies --- Cosmochronology. --- Étoiles des premiers types. --- Étoiles --- Étoiles --- Galaxies --- Cosmochronologie. --- Voie lactée. --- Age. --- Formation. --- Formation. --- Age. --- Formation. --- Formation. --- Milky Way.
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In this work, the emphasis will be placed on the understating of the theory needed to try to describe correctly the interaction between convection and pulsation. We will shed light on important terms appearing due to turbulent flows and see how we can describe them. Hence, we will present more evolved models that should reproduce the reality with a better fidelity. Finally, to illustrate and compare the different possible models introduced previously, we will study a well-known type of variable stars: the ZZ Ceti white dwarfs. These dying stars are known for their extremely thin but efficient convection envelope (as most white dwarfs) and for their instability strip for which better predictions are still needed in order to match the observations. Dans ce travail, l'emphase sera mise sur la compréhension de la théorie nécessaire pour décrire correctement l’interaction entre la convection et les pulsations. Nous mettrons en évidence l'apparition de termes importants supplémentaires provenant des écoulements turbulents et nous verrons comment ils peuvent être décrits. De plus, nous présenterons des modèles plus évolués censés reproduire la réalité avec une meilleure fidélité. Finalement, pour illustrer et comparer les différents modèles que nous auront préalablement introduits, nous étudierons un type d'étoiles variables bien connu : les naines blanches ZZ Ceti. Ces étoiles en fin de vie sont connues pour leur enveloppe convective fine mais très importante et surtout pour leur bande d'instabilité pour laquelle de meilleures prédictions sont toujours nécessaires afin de reproduire les observations.
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