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010   $a3-319-18772-4
024 7 $a10.1007/978-3-319-18772-3
035   $a(CKB)3710000000434206
035   $a(EBL)2120640
035   $a(OCoLC)911179603
035   $a(SSID)ssj0001525198
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035   $a(PQKBTitleCode)TC0001525198
035   $a(PQKBWorkID)11496987
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035   $a(DE-He213)978-3-319-18772-3
035   $a(MiAaPQ)EBC2120640
035   $a(PPN)18640140X
035   $a(EXLCZ)993710000000434206
100   $a20150615d2015      u|         0
101 0 $aeng
135   $aur|n|---|||||
181   $ctxt
182   $cc
183   $acr
200 10$aDynamics of the Milky Way $eTidal Streams and Extended Distribution Functions for the Galactic Disc /$fby Jason Sanders
205   $a1st ed. 2015.
210  1$aCham :$cSpringer International Publishing :$cImprint: Springer,$d2015.
215   $a1 online resource (274 p.)
225 1 $aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
300   $aDescription based upon print version of record.
311   $a3-319-18771-6 
320   $aIncludes bibliographical references.
327   $aIntroduction -- Angle-Action Estimation in a General Axisymmetric Potential -- Actions, Angles and Frequencies from Numerically Integrated Orbits -- Action Estimation Using a Triaxial Stäckel Approximation -- Stream-Orbit Misalignment -- Stream Modelling in Angle-Frequency Space -- Determining the Velocity Dispersion of the Thick Disc -- Extended Distribution Functions for the Galactic Disc -- Conclusions.
330   $aThis work presents a study of methods useful for modeling and understanding dynamical systems in the Galaxy. A natural coordinate system for the study of dynamical systems is the angle-action coordinate system. New methods for the approximation of the action-angle variables in general potentials are presented and discussed. These new tools are applied to the construction of dynamical models for two of the Galaxy?s components: tidal streams and the Galactic disc. Tidal streams are remnants of tidally stripped satellites in the Milky Way that experience the effects of the large scale structure of the Galactic gravitational potential, while the Galactic disc provides insights into the nature of the Galaxy near the Sun. Appropriate action-based models are presented and discussed for these components, and extended to include further information such as the metallicity of stars.
410  0$aSpringer Theses, Recognizing Outstanding Ph.D. Research,$x2190-5053
606   $aSpace sciences
606   $aMathematical physics
606   $aStatistical physics
606   $aDynamics
606   $aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics)$3https://scigraph.springernature.com/ontologies/product-market-codes/P22030
606   $aTheoretical, Mathematical and Computational Physics$3https://scigraph.springernature.com/ontologies/product-market-codes/P19005
606   $aComplex Systems$3https://scigraph.springernature.com/ontologies/product-market-codes/P33000
606   $aStatistical Physics and Dynamical Systems$3https://scigraph.springernature.com/ontologies/product-market-codes/P19090
615  0$aSpace sciences.
615  0$aMathematical physics.
615  0$aStatistical physics.
615  0$aDynamics.
615 14$aSpace Sciences (including Extraterrestrial Physics, Space Exploration and Astronautics).
615 24$aTheoretical, Mathematical and Computational Physics.
615 24$aComplex Systems.
615 24$aStatistical Physics and Dynamical Systems.
676   $a523.113
700   $aSanders$b Jason$4aut$4http://id.loc.gov/vocabulary/relators/aut$0323318
801  0$bMiAaPQ
801  1$bMiAaPQ
801  2$bMiAaPQ
906   $aBOOK
912   $a9910300408103321
996   $aDynamics of the Milky Way$91771540
997   $aUNINA