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Probing galaxy evolution by unveiling the structure of massive galaxies across cosmic time and in diverse environments[electronic resource] /

紀錄類型:	書目-語言資料,印刷品 : Monograph/item
杜威分類號:	523.112
書名/作者:	Probing galaxy evolution by unveiling the structure of massive galaxies across cosmic time and in diverse environments/ by Timothy Weinzirl.
作者:	Weinzirl, Timothy.
出版者:	Cham : : Springer International Publishing :, 2015.
面頁冊數:	xiv, 236 p. : : ill. (some col.), digital ;; 24 cm.
Contained By:	Springer eBooks
標題:	Galaxies - Evolution.
標題:	Galaxies - Formation.
標題:	Physics.
標題:	Astronomy, Astrophysics and Cosmology.
標題:	Cosmology.
ISBN:	9783319069593 (electronic bk.)
ISBN:	9783319069586 (paper)
內容註:	Introduction -- Probing the Structure and Assembly of Nearby Field Spirals -- Exploring the Structure and Assembly of Galaxies at the Heart of the Coma Cluster -- Structure and Assembly of the Most Massive Galaxies Present a Few Gyr (z~ 2 - 3) After the Big Bang -- Summary, Implications and Future Work.
摘要、提要註:	Awarded the American Astronomical Society (AAS) Rodger Doxsey Travel Prize, and with a foreword by thesis supervisor Professor Shardha Jogee at the University of Texas at Austin, this thesis discusses one of the primary outstanding problems in extragalactic astronomy: how galaxies form and evolve. Galaxies consist of two fundamental kinds of structure: rotationally supported disks and spheroidal/triaxial structures supported by random stellar motions. Understanding the balance between these galaxy components is vital to comprehending the relative importance of the different mechanisms (galaxy collisions, gas accretion and internal secular processes) that assemble and shape galaxies. Using panchromatic imaging from some of the largest and deepest space-based galaxy surveys, an empirical census of galaxy structure is made for galaxies at different cosmic epochs and in environments spanning low to extremely high galaxy number densities. An important result of this work is that disk structures are far more prevalent in massive galaxies than previously thought. The associated challenges raised for contemporary theoretical models of galaxy formation are discussed. The method of galaxy structural decomposition is treated thoroughly since it is relevant for future studies of galaxy structure using next-generation facilities, like the James Webb Space Telescope and the ground-based Giant Magellan Telescope with adaptive optics.
電子資源:	http://dx.doi.org/10.1007/978-3-319-06959-3

Probing galaxy evolution by unveiling the structure of massive galaxies across cosmic time and in diverse environments[electronic resource] /
Weinzirl, Timothy.

Probing galaxy evolution by unveiling the structure of massive galaxies across cosmic time and in diverse environments[electronic resource] /by Timothy Weinzirl. - Cham :Springer International Publishing :2015. - xiv, 236 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- Probing the Structure and Assembly of Nearby Field Spirals -- Exploring the Structure and Assembly of Galaxies at the Heart of the Coma Cluster -- Structure and Assembly of the Most Massive Galaxies Present a Few Gyr (z~ 2 - 3) After the Big Bang -- Summary, Implications and Future Work.

Awarded the American Astronomical Society (AAS) Rodger Doxsey Travel Prize, and with a foreword by thesis supervisor Professor Shardha Jogee at the University of Texas at Austin, this thesis discusses one of the primary outstanding problems in extragalactic astronomy: how galaxies form and evolve. Galaxies consist of two fundamental kinds of structure: rotationally supported disks and spheroidal/triaxial structures supported by random stellar motions. Understanding the balance between these galaxy components is vital to comprehending the relative importance of the different mechanisms (galaxy collisions, gas accretion and internal secular processes) that assemble and shape galaxies. Using panchromatic imaging from some of the largest and deepest space-based galaxy surveys, an empirical census of galaxy structure is made for galaxies at different cosmic epochs and in environments spanning low to extremely high galaxy number densities. An important result of this work is that disk structures are far more prevalent in massive galaxies than previously thought. The associated challenges raised for contemporary theoretical models of galaxy formation are discussed. The method of galaxy structural decomposition is treated thoroughly since it is relevant for future studies of galaxy structure using next-generation facilities, like the James Webb Space Telescope and the ground-based Giant Magellan Telescope with adaptive optics.

ISBN: 9783319069593 (electronic bk.)

Standard No.: 10.1007/978-3-319-06959-3doiSubjects--Topical Terms:

467749
Galaxies
--Evolution.

LC Class. No.: QB857.5.E96

Dewey Class. No.: 523.112

Probing galaxy evolution by unveiling the structure of massive galaxies across cosmic time and in diverse environments[electronic resource] /
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