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Astrophysical Disks: Collective and Stochastic Phenomena (2006)

Astrophysical Disks

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"Astrophysical Disks" by Aleksey M. Fridman, Mikhail Ya. Marov, Ilya G. Kovalenko is a mathematics book and learning resource focused on Deep Sky & Solar System. Best for teachers, students, and readers looking for stronger mathematical understanding.

The book deals with collective and stochastic processes in astrophysical discs involving theory, observations, and the results of modelling. Among others, it examines the spiral-vortex structure in galactic and accretion disks, stochastic and ordered structures in the developed turbulence. It also describes sources of turbulence in the accretion disks, internal structure of disk in the vicinity of a black hole, numerical modelling of Be envelopes in binaries, gaseous disks in spiral galaxies with shock waves formation, observation of accretion disks in a binary system and mass distribution of luminous matter in disk galaxies.

The editors adaptly brought together collective and stochastic phenomena in the modern field of astrophysical discs, their formation, structure, and evolution involving the methodology to deal with, the results of observation and modelling, thereby advancing the study in this important branch of astrophysics and benefiting Professional Researchers, Lecturers, and Graduate Students.

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Best For: Professional researchers, lecturers, and graduate students in astrophysics and related fields
Focus: Collective and stochastic processes in astrophysical disks, including theory, observations, and modeling
Covers: Spiral-vortex structures in galactic and accretion disks, turbulence sources, internal disk structure near black holes, numerical modeling of Be envelopes in binaries, gaseous disks in spiral galaxies with shock waves, accretion disk observations in binar
Why It Matters: Provides a comprehensive approach combining theory, observation, and modeling to advance understanding of formation, structure, and evolution of astrophysical disks

"Astrophysical Disks" by Aleksey M. Fridman, Mikhail Ya. Marov, Ilya G. Kovalenko is a mathematics book and learning resource focused on Deep Sky & Solar System. Best for teachers, students, and readers looking for stronger mathematical understanding.

Topic: Deep Sky & Solar System

Author: Aleksey M. Fridman, Mikhail Ya. Marov, Ilya G. Kovalenko

Who this is for:

  • Teachers and classroom instructors
  • Students building subject mastery
  • Readers looking for practical learning support

Why this book matters: It stands out as a practical math resource that helps explain concepts, strengthen problem-solving, and support classroom or independent learning.

The book deals with collective and stochastic processes in astrophysical discs involving theory, observations, and the results of modelling. Among others, it examines the spiral-vortex structure in galactic and accretion disks, stochastic and ordered structures in the developed turbulence. It also describes sources of turbulence in the accretion disks, internal structure of disk in the vicinity of a black hole, numerical modelling of Be envelopes in binaries, gaseous disks in spiral galaxies with shock waves formation, observation of accretion disks in a binary system and mass distribution of luminous matter in disk galaxies.

The editors adaptly brought together collective and stochastic phenomena in the modern field of astrophysical discs, their formation, structure, and evolution involving the methodology to deal with, the results of observation and modelling, thereby advancing the study in this important branch of astrophysics and benefiting Professional Researchers, Lecturers, and Graduate Students.

AuthorAleksey M. Fridman, Mikhail Ya. Marov, Ilya G. Kovalenko
PublisherSpringer
Published2006-06-26
ISBN-139781402043475
BindingPaperback
Pages358
LanguageEnglish
SubjectsScience
TopicDeep Sky & Solar System
SeriesAstrophysics and Space Science Library

Format: Paperback

Length: 358 pages

Language: English

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