Stellar Rotation (Cambridge Astrophysics)

by Jean-Louis Tassoul

Publisher: Cambridge University Press

Written in English
Cover of: Stellar Rotation (Cambridge Astrophysics) | Jean-Louis Tassoul
Published: Pages: 272 Downloads: 720
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Subjects:

  • Astrophysics,
  • Solar system,
  • Stars, interstellar matter,
  • Science,
  • Science/Mathematics,
  • Astronomy - Universe,
  • Science / Astrophysics & Space Science,
  • Science : Astronomy - Universe,
  • Stars--Rotation,
  • Astrophysics & Space Science,
  • Proper motion,
  • Stars
The Physical Object
FormatPaperback
Number of Pages272
ID Numbers
Open LibraryOL7715354M
ISBN 100521037697
ISBN 109780521037693

Book Description: Ever since the first observations of sunspots in the early seventeenth century, stellar rotation has been a major topic in astronomy and astrophysics. Jean-Louis Tassoul . His indistinct stellar energy rushes forth and forms a maelstrom-like nebula around his body. At the same time, a stream of his Stellar Flame enfolds the yuanying and begins to gradually melt it and get rid of the impurities. The energy of the yuanying then starts to move according to the rotation of the maelstrom of stellar . Stellar Evolution - CRC Press Book This book addresses the fascinating subject of astrophysics from its theoretical basis to predominant research conducted in the field today. An . “Modes of oscillation that propagate in the direction of rotation move faster than the modes that propagate in the opposite direction, thus their frequencies are slightly different,” he said. “Our best measurements all reveal stars with solar-like rotation.” The research shows the potential of asteroseismology for probing stellar .

  Gregory Simonian, graduate student at Ohio State, presented “Double Trouble: Biases Caused by Binaries in Large Stellar Rotation datasets”. The Kepler data yiel rotation . Each chapter is written by leading experts in the field, and the book provides an overview that is central to any attempt to understand the properties of stars and their evolution. With extensive references to the technical literature, this is a valuable text for researchers and graduate students in stellar . Stellar rotation is the angular motion of a star about its axis. The rate of rotation can be measured from the spectrum of the star, or by timing the movements of active features on the surface. The rotation of a star produces an equatorial bulge due to centripetal force. As stars are not solid bodies, they can also undergo differential rotation. In astronomy, the Kraft break refers to the abrupt decrease in stars' average rotation rates at surface temperatures of about kelvin. The so-called break was first noted by the .

  Theory of Stellar Atmospheres: An Introduction to Astrophysical Non-equilibrium Quantitative Spectroscopic Analysis - Ebook written by Ivan Hubeny, Dimitri Mihalas. Read this book using Google Play Books app on your PC, android, iOS devices. Download for offline reading, highlight, bookmark or take notes while you read Theory of Stellar 5/5(1).

Stellar Rotation (Cambridge Astrophysics) by Jean-Louis Tassoul Download PDF EPUB FB2

Buy Stellar Rotation (Cambridge Astrophysics) on FREE SHIPPING on qualified orders Stellar Rotation (Cambridge Astrophysics): Jean-Louis Tassoul: : Books.

Buy Stellar Rotation (Cambridge Astrophysics) on FREE SHIPPING on qualified orders Stellar Rotation (Cambridge Astrophysics): Tassoul, Jean-Louis: : Books. Provides the fundamentals of astroseismology with a focus on waves caused by stellar rotation and by stellar convection.

Gives the necessary theoretical background to interpret. This book will be of primary interest to graduate students and researchers studying solar and stellar rotation and close binary systems. It will also appeal to those with a more general interest in solar and stellar Price Range: £ - £ This book will be of primary interest to graduate students and researchers studying solar and stellar rotation and close binary systems.

It will also appeal to those with a more general interest in solar and stellar. The International Astronomical Union Colloquium on Stellar Rotation was held Stellar Rotation book the Ohio State University in Columbus, Ohio, U.S.A.

from September 8th through 11 th, Forty-four. The chapters in this book address Stellar Rotation book two groups of topics summarized as "Stellar Rotation and Associated Seismology" as well as "Stellar Convection and Associated Seismology". The book Brand: Springer Berlin Heidelberg.

Axial rotation along the upper main sequence Circulation, rotation, and diffusion Rotation of evolved stars Bibliographical notes 7 The late-type stars Introduction Schatzman’s braking mechanism Rotation File Size: KB.

The chapters in this book address the two groups of topics summarized as "Stellar Rotation and Associated Seismology" as well as "Stellar Convection and Associated Seismology". The book Brand: Springer Berlin Heidelberg. The present book provides an introduction to techniques and analyses used in observing stellar photospheres.

Fourier transforms are examined, and instruments employed for photospheric Cited by: Download Book online More book More Links. Download Book online More book More Links. Search this site. Home. 4th Panzer Division on the Eastern Front: v. 1 (Armor at. Understanding how stars rotate is central to modelling their structure, formation, and evolution and how they interact with their environment and companion stars.

This authoritative volume provides a lucid introduction to stellar rotation. The chapters in this book address the two groups of topics summarized as "Stellar Rotation and Associated Seismology" as well as "Stellar Convection and Associated Seismology".

The book Pages: Rotation induces instabilities which in turn induce mixing. The mixing leads to larger cores and longer lifetimes, and also modifies the nucleosynthesis.

For the most massive stars, fast rotation. It combines theory and observation in a comprehensive survey of how the rotation of stars affects the structure and evolution of the Sun, single stars, and close binaries.

This timely book will be of primary interest to graduate students and researchers studying solar and stellar rotation. item 2 Stellar Rotation by Jean Louis Tassoul (English) Paperback Book Free Shipping.

- Stellar Rotation by Jean Louis Tassoul (English) Paperback Book Free Shipping. $ Free. The measurement of stellar continua; The line absorption coefficient; The measurement of spectral lines; The behavior of spectral lines; The measurement of stellar radii and temperatures; The measurement of photospheric pressure; Chemical analysis; Velocity fields in stellar photospheres; Stellar : David F.

Gray. The rotation of stars has many interesting and important consequences for the photometric and chemical evolution of galaxies.

Many of the predictions of models of stellar rotation are now. This book brings together for the first time recent results in solar studies and stellar studies. The result is an illuminating new view of stellar magnetic activity.

Key topics include radiative transfer, convective simulations, dynamo theory, outer-atmospheric heating, stellar 5/5(1). Purchase Stellar Formation - 1st Edition. Print Book & E-Book. ISBNBook Edition: 1. In: Stellar astrophysical fluid dynamics.

Edited by Michael J. Thompson, Jørgen Christensen-Dalsgaard. Cambridge (UK): Cambridge University Press, ISBN, p. 75 - Figure Using a Spectrum to Determine Stellar Rotation.

A rotating star will show broader spectral lines than a nonrotating star. Measurements of the widths of spectral lines show that. The text first discusses the fundamentals concepts of stellar statistics, and then proceeds to detailing the kinematics of stellar systems.

The next chapter covers the elementary theory of galactic rotation. Next, the book tackles the irregular forces in stellar systems. Chapter V talks about the statistical stellar. Stellar rotation and magnetic stars axis to the line of sight is not in general known, what is measured is the projected rotation speed v sin i rather than the actual equatorial rotation Cited by: Jean-Louis and Monique Tassoul received the Paul and Marie Stroobant Prize of the Académie Royale de Belgique for their work on stellar rotation and stellar stability.

From toJean-Louis, whose books 5/5(2). Stellar Spectroscopy is the study of the spectra of starlight. Astrophysicists can use this effect to calculate the stellar rotation rate. For simplicity lets assume that the axis of rotation is.

Why can only a lower limit to the rate of stellar rotation be determined from line broadening rather than the actual rotation rate. (Refer to Figure ). Reference. The chapter discusses photometry, spectroscopy, magnetic activity, heated regions of the atmospheres, and mass and angular momentum loss.

Observing other stars provides a window into the behavior of solar-type stars with a wide range of masses, ages, rotation rates, and other stellar Author: Gibor Basri. ADS Classic is now deprecated.

It will be completely retired in October Please redirect your searches to the new ADS modern form or the classic info can be found on our blog. This book, while not attempting to answer all questions about rotation, given that many issues still have to be further investigated, focuses on the basics and some particular aspects while aiming to show why it is important, from a physical point of view, to study stellar rotation.

'Understanding Stellar Evolution' is based on a series of graduate-level courses taught at the University of Washington sinceand is written for physics and astronomy students and .Rotation is an important physical process that can have a significant impact on stellar ev olution (see e.g.

[ 1 ]). Rotational effects have generally been included in stellar ev olution codes in.Our Galaxy - The Milky Way •Overall structure and major components •The concept of stellar populations •Stellar kinematics •Galactic rotation and the evidence for a dark halo •Galactic .