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Modeling and analysis of eclipsing binary stars : the theory and design principles of PHOEBE /

The fascinating and observationally spectacular world of binary stars is a vast and beautiful one that is a significant aspect of many astrophysical studies. Modeling and Analysis of Eclipsing Binary Stars gives a comprehensive analysis and description of the science behind eclipsing binaries. It al...

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Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Prša, Andrej (Autor)
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Bristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) : IOP Publishing, [2018]
Colección:IOP (Series). Release 5.
AAS-IOP astronomy. Release 1.
Temas:
Acceso en línea:Texto completo

MARC

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020 |z 9780750312882  |q print 
024 7 |a 10.1088/978-0-7503-1287-5  |2 doi 
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100 1 |a Prša, Andrej,  |e author. 
245 1 0 |a Modeling and analysis of eclipsing binary stars :  |b the theory and design principles of PHOEBE /  |c Andrej Prša. 
246 3 0 |a Theory and design principles of PHOEBE. 
264 1 |a Bristol [England] (Temple Circus, Temple Way, Bristol BS1 6HG, UK) :  |b IOP Publishing,  |c [2018] 
300 |a 1 online resource (various pagings) :  |b illustrations (some color). 
336 |a text  |2 rdacontent 
337 |a electronic  |2 isbdmedia 
338 |a online resource  |2 rdacarrier 
490 1 |a [IOP release 5] 
490 1 |a AAS-IOP astronomy. [release 1],  |x 2514-3433 
500 |a "Version: 20181201"--Title page verso. 
504 |a Includes bibliographical references. 
505 0 |a 1. Introduction to the field -- 1.1. Why binaries are important -- 1.2. Why eclipsing binaries are even more important 
505 8 |a part I. Observations. 2. Observations and data acquisition -- 2.1. Timekeeping -- 2.2. Photometry -- 2.3. Spectroscopy -- 2.4. Interferometry -- 2.5. Astrometry -- 2.6. Polarimetry -- 2.7. Asteroseismology 
505 8 |a part II. Theoretical background. 3. Geometry and dynamics of binary stars -- 3.1. A quick look at the Roche model -- 3.2. Roche model generalization -- 3.3. Orbital properties of close binaries -- 3.4. Dynamical aspects of binary systems 
505 8 |a 4. Radiation : the basics -- 4.1. Intensity -- 4.2. Flux -- 4.3. Luminosity -- 4.4. Limb darkening -- 4.5. Computational efficiency -- 4.6. Relative units -- 4.7. Blackbody radiation -- 4.8. Putting it all together 
505 8 |a 5. Radiative properties of binary stars -- 5.1. Gravity darkening -- 5.2. Reflection effect -- 5.3. Stellar spots -- 5.4. Doppler boosting -- 5.5. Interstellar and atmospheric extinction 
505 8 |a 6. Advanced topics -- 6.1. Misaligned stellar rotation axes -- 6.2. Multiple systems -- 6.3. Granulation -- 6.4. Color indices and effective temperatures -- 6.5. Limitations 
505 8 |a part III. Modeling considerations. 7. Numerical model -- 7.1. Discretization of stellar surfaces -- 7.2. Dynamical aspects -- 7.3. Computation of local geometric quantities -- 7.4. Computation of local radiative quantities -- 7.5. Computation of aspect-dependent quantities 
505 8 |a 8. Approaches to solving the inverse problem -- 8.1. Local and global minima in the parameter hyperspace -- 8.2. Differential corrections -- 8.3. Powell's direction set method -- 8.4. Nelder & Mead's downhill simplex method -- 8.5. Adaptive simulated annealing -- 8.6. Formal errors of the fit -- 8.7. Handling degeneracies efficiently -- 8.8. Markov chain Monte Carlo samplers -- 8.9. Parameter constraints as degeneracy breakers -- 9. Conclusion. 
520 3 |a The fascinating and observationally spectacular world of binary stars is a vast and beautiful one that is a significant aspect of many astrophysical studies. Modeling and Analysis of Eclipsing Binary Stars gives a comprehensive analysis and description of the science behind eclipsing binaries. It also explores the assumptions and the difficulties that can occur when using the modeling principles of the classical codes as well as introducing PHOEBE (the PHysics Of Eclipsing BinariEs)--a modern suite for modeling binary stars. PHOEBE was conceived by Andrej Prša and his collaborators, and has become one of the standard tools in the eclipsing binary field. 
530 |a Also available in print. 
538 |a Mode of access: World Wide Web. 
538 |a System requirements: Adobe Acrobat Reader, EPUB reader, or Kindle reader. 
545 |a Andrej Prša is a Slovenian astrophysicist who obtained his PhD in physics from the University of Ljubljana in 2005. The principal result of his doctoral thesis was PHOEBE (PHysics Of Eclipsing BinariEs), a modeling suite for binary stars that has since become one of the standards in the binary star community. Prša is passionate about his subject and he is a dedicated teacher and astrophysicist whose research and work is a huge asset to the astronomical community. 
588 0 |a Title from PDF title page (viewed on January 16, 2019). 
650 0 |a Eclipsing binaries. 
650 0 |a Eclipsing binaries  |x Light curves. 
650 7 |a Galaxies & stars.  |2 bicssc 
650 7 |a SCIENCE / Astronomy.  |2 bisacsh 
710 2 |a Institute of Physics (Great Britain),  |e publisher. 
776 0 8 |i Print version:  |z 9780750312882 
830 0 |a IOP (Series).  |p Release 5. 
830 0 |a AAS-IOP astronomy.  |p Release 1. 
856 4 0 |u https://iopscience.uam.elogim.com/book/978-0-7503-1287-5  |z Texto completo