國立高雄大學圖資館 |

語系: 繁體中文

說明(常見問題)

圖資館首頁

登入

回首頁

切換: 標籤 | MARC模式 | ISBD

Dynamics of the Milky Waytidal strea...

Milky Way.

Dynamics of the Milky Waytidal streams and extended distribution functions for the galactic disc /

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	Dynamics of the Milky Wayby Jason Sanders.
其他題名:	tidal streams and extended distribution functions for the galactic disc /
作者:	Sanders, Jason.
出版者:	Cham :Springer International Publishing :2015.
面頁冊數:	xxii, 264 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
標題:	Galactic dynamics.
標題:	Milky Way.
電子資源:	http://dx.doi.org/10.1007/978-3-319-18772-3
ISBN:	9783319187723 (electronic bk.)

Dynamics of the Milky Waytidal streams and extended distribution functions for the galactic disc /
Sanders, Jason.

Dynamics of the Milky Waytidal streams and extended distribution functions for the galactic disc /[electronic resource] :by Jason Sanders. - Cham :Springer International Publishing :2015. - xxii, 264 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- Angle-Action Estimation in a General Axisymmetric Potential -- Actions, Angles and Frequencies from Numerically Integrated Orbits -- Action Estimation Using a Triaxial Stackel 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.

This 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.

ISBN: 9783319187723 (electronic bk.)

Standard No.: 10.1007/978-3-319-18772-3doiSubjects--Topical Terms:

727030
Galactic dynamics.
Subjects--Geographical Terms:

560752
Milky Way.

LC Class. No.: QB857.7

Dewey Class. No.: 523.113

Dynamics of the Milky Waytidal streams and extended distribution functions for the galactic disc /
LDR:02326nmm a2200325 a 4500 001 471648
003 DE-He213
005 20160126141548.0
006 m d
007 cr nn 008maaau
008 160223s2015 gw s 0 eng d
020 $a 9783319187723 (electronic bk.)
020 $a 9783319187716 (paper)
024 7 $a 10.1007/978-3-319-18772-3 $2 doi
035 $a 978-3-319-18772-3
040 $a GP $c GP
041 0 $a eng
050 4 $a QB857.7
072 7 $a TTDS $2 bicssc
072 7 $a SCI005000 $2 bisacsh
082 0 4 $a 523.113 $2 23
090 $a QB857.7 $b .S215 2015
100 1 $a Sanders, Jason. $3 727029
245 1 0 $a Dynamics of the Milky Way $h [electronic resource] : $b tidal streams and extended distribution functions for the galactic disc / $c by Jason Sanders.
260 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2015.
300 $a xxii, 264 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a Introduction -- Angle-Action Estimation in a General Axisymmetric Potential -- Actions, Angles and Frequencies from Numerically Integrated Orbits -- Action Estimation Using a Triaxial Stackel 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.
520 $a This 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.
650 0 $a Galactic dynamics. $3 727030
650 1 4 $a Physics. $3 179414
650 2 4 $a Extraterrestrial Physics, Space Sciences. $3 274037
650 2 4 $a Theoretical, Mathematical and Computational Physics. $3 376743
650 2 4 $a Statistical Physics, Dynamical Systems and Complexity. $3 376808
651 0 $a Milky Way. $3 560752
710 2 $a SpringerLink (Online service) $3 273601
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 557607
856 4 0 $u http://dx.doi.org/10.1007/978-3-319-18772-3
950 $a Physics and Astronomy (Springer-11651)