國立高雄大學圖資館 |

Language: English

Back

A statistical and multi-wavelength s...

Schreiber, Corentin.

A statistical and multi-wavelength study of star formation in galaxies

Record Type:	Electronic resources : Monograph/item
Title/Author:	A statistical and multi-wavelength study of star formation in galaxiesby Corentin Schreiber.
Author:	Schreiber, Corentin.
Published:	Cham :Springer International Publishing :2016.
Description:	xvii, 218 p. :ill., digital ;24 cm.
Contained By:	Springer eBooks
Subject:	GalaxiesFormation.
Online resource:	http://dx.doi.org/10.1007/978-3-319-44293-8
ISBN:	9783319442938$q(electronic bk.)

A statistical and multi-wavelength study of star formation in galaxies
Schreiber, Corentin.

A statistical and multi-wavelength study of star formation in galaxies[electronic resource] /by Corentin Schreiber. - Cham :Springer International Publishing :2016. - xvii, 218 p. :ill., digital ;24 cm. - Springer theses,2190-5053. - Springer theses..

Introduction -- Summary of the Work Done in This Thesis -- Modelling the Integrated IR Photometry of Star-forming Galaxies -- Gencat: An Empirical Simulation of the Observable Universe -- The Downfall of Massive Star-Forming Galaxies During the Last 10 Gyr -- Reaching the Distant Universe with ALMA -- Conclusions and Perspectives.

This thesis presents a pioneering method for gleaning the maximum information from the deepest images of the far-infrared universe obtained with the Herschel satellite, reaching galaxies fainter by an order of magnitude than in previous studies. Using these high-quality measurements, the author first demonstrates that the vast majority of galaxy star formation did not take place in merger-driven starbursts over 90% of the history of the universe, which suggests that galaxy growth is instead dominated by a steady infall of matter. The author further demonstrates that massive galaxies suffer a gradual decline in their star formation activity, providing an alternative path for galaxies to stop star formation. One of the key unsolved questions in astrophysics is how galaxies acquired their mass in the course of cosmic time. In the standard theory, the merging of galaxies plays a major role in forming new stars. Then, old galaxies abruptly stop forming stars through an unknown process. Investigating this theory requires an unbiased measure of the star formation intensity of galaxies, which has been unavailable due to the dust obscuration of stellar light.

ISBN: 9783319442938$q(electronic bk.)

Standard No.: 10.1007/978-3-319-44293-8doiSubjects--Topical Terms:

267028
Galaxies
--Formation.

LC Class. No.: QB857

Dewey Class. No.: 523.112

A statistical and multi-wavelength study of star formation in galaxies
LDR:02493nmm a2200325 a 4500 001 497659
003 DE-He213
005 20170314151941.0
006 m d
007 cr nn 008maaau
008 170420s2016 gw s 0 eng d
020 $a 9783319442938$q(electronic bk.)
020 $a 9783319442921$q(paper)
024 7 $a 10.1007/978-3-319-44293-8 $2 doi
035 $a 978-3-319-44293-8
040 $a GP $c GP
041 0 $a eng
050 4 $a QB857
072 7 $a PHVB $2 bicssc
072 7 $a SCI005000 $2 bisacsh
082 0 4 $a 523.112 $2 23
090 $a QB857 $b .S378 2016
100 1 $a Schreiber, Corentin. $3 760431
245 1 2 $a A statistical and multi-wavelength study of star formation in galaxies $h [electronic resource] / $c by Corentin Schreiber.
260 $a Cham : $b Springer International Publishing : $b Imprint: Springer, $c 2016.
300 $a xvii, 218 p. : $b ill., digital ; $c 24 cm.
490 1 $a Springer theses, $x 2190-5053
505 0 $a Introduction -- Summary of the Work Done in This Thesis -- Modelling the Integrated IR Photometry of Star-forming Galaxies -- Gencat: An Empirical Simulation of the Observable Universe -- The Downfall of Massive Star-Forming Galaxies During the Last 10 Gyr -- Reaching the Distant Universe with ALMA -- Conclusions and Perspectives.
520 $a This thesis presents a pioneering method for gleaning the maximum information from the deepest images of the far-infrared universe obtained with the Herschel satellite, reaching galaxies fainter by an order of magnitude than in previous studies. Using these high-quality measurements, the author first demonstrates that the vast majority of galaxy star formation did not take place in merger-driven starbursts over 90% of the history of the universe, which suggests that galaxy growth is instead dominated by a steady infall of matter. The author further demonstrates that massive galaxies suffer a gradual decline in their star formation activity, providing an alternative path for galaxies to stop star formation. One of the key unsolved questions in astrophysics is how galaxies acquired their mass in the course of cosmic time. In the standard theory, the merging of galaxies plays a major role in forming new stars. Then, old galaxies abruptly stop forming stars through an unknown process. Investigating this theory requires an unbiased measure of the star formation intensity of galaxies, which has been unavailable due to the dust obscuration of stellar light.
650 0 $a Galaxies $x Formation. $3 267028
650 1 4 $a Physics. $3 179414
650 2 4 $a Astrophysics and Astroparticles. $3 376943
650 2 4 $a Numerical and Computational Physics, Simulation. $3 758154
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/10.1007/978-3-319-44293-8
950 $a Physics and Astronomy (Springer-11651)