語系:
繁體中文
English
說明(常見問題)
圖資館首頁
登入
回首頁
切換:
標籤
|
MARC模式
|
ISBD
Morphology, kinematics and star form...
~
Erroz-Ferrer, Santiago.
Morphology, kinematics and star formation across the Hubble sequence of galaxies
紀錄類型:
書目-電子資源 : Monograph/item
正題名/作者:
Morphology, kinematics and star formation across the Hubble sequence of galaxiesby Santiago Erroz-Ferrer.
作者:
Erroz-Ferrer, Santiago.
出版者:
Cham :Springer International Publishing :2016.
面頁冊數:
xiii, 201 p. :ill. (some col.), digital ;24 cm.
Contained By:
Springer eBooks
標題:
Physics.
電子資源:
http://dx.doi.org/10.1007/978-3-319-26398-4
ISBN:
9783319263984$q(electronic bk.)
Morphology, kinematics and star formation across the Hubble sequence of galaxies
Erroz-Ferrer, Santiago.
Morphology, kinematics and star formation across the Hubble sequence of galaxies
[electronic resource] /by Santiago Erroz-Ferrer. - Cham :Springer International Publishing :2016. - xiii, 201 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5053. - Springer theses..
Introduction -- Massive star formation in galaxies with excess UV emission -- H_ kinematics of S4G spiral galaxies: The data -- Streaming motions in the spiral galaxy NGC 864 -- Non-circular motions and star formation in S4G galaxies -- Inner rotation curves -- Conclusions and future work.
This thesis discusses the evolution of galaxies through the study of the morphology, kinematics, and star formation properties of a sample of nearby galaxies. The main body of the thesis describes the kinematic observations with the GHaFAS Fabry-Perot instrument on the William Herschel Telescope of a sample of 29 spiral galaxies. The work is closely related to the Spitzer Survey of Stellar Structure in Galaxies, and uses the mid-infrared data of that survey to determine key parameters of the galaxies studied. From these data, important results are obtained on streaming and other non-circular motions in galaxies, on the distribution and rates of star formation, and on how correlations of these parameters and of the rotation curve shape with basic galaxy parameters yield clues on the evolutionary processes taking place in disk galaxies.
ISBN: 9783319263984$q(electronic bk.)
Standard No.: 10.1007/978-3-319-26398-4doiSubjects--Topical Terms:
179414
Physics.
LC Class. No.: QB4
Dewey Class. No.: 520
Morphology, kinematics and star formation across the Hubble sequence of galaxies
LDR
:02178nmm a2200337 a 4500
001
482006
003
DE-He213
005
20160801165538.0
006
m d
007
cr nn 008maaau
008
161007s2016 gw s 0 eng d
020
$a
9783319263984$q(electronic bk.)
020
$a
9783319263977$q(paper)
024
7
$a
10.1007/978-3-319-26398-4
$2
doi
035
$a
978-3-319-26398-4
040
$a
GP
$c
GP
041
0
$a
eng
050
4
$a
QB4
072
7
$a
PG
$2
bicssc
072
7
$a
SCI004000
$2
bisacsh
072
7
$a
NAT033000
$2
bisacsh
082
0 4
$a
520
$2
23
090
$a
QB4
$b
.E72 2016
100
1
$a
Erroz-Ferrer, Santiago.
$3
738416
245
1 0
$a
Morphology, kinematics and star formation across the Hubble sequence of galaxies
$h
[electronic resource] /
$c
by Santiago Erroz-Ferrer.
260
$a
Cham :
$b
Springer International Publishing :
$b
Imprint: Springer,
$c
2016.
300
$a
xiii, 201 p. :
$b
ill. (some col.), digital ;
$c
24 cm.
490
1
$a
Springer theses,
$x
2190-5053
505
0
$a
Introduction -- Massive star formation in galaxies with excess UV emission -- H_ kinematics of S4G spiral galaxies: The data -- Streaming motions in the spiral galaxy NGC 864 -- Non-circular motions and star formation in S4G galaxies -- Inner rotation curves -- Conclusions and future work.
520
$a
This thesis discusses the evolution of galaxies through the study of the morphology, kinematics, and star formation properties of a sample of nearby galaxies. The main body of the thesis describes the kinematic observations with the GHaFAS Fabry-Perot instrument on the William Herschel Telescope of a sample of 29 spiral galaxies. The work is closely related to the Spitzer Survey of Stellar Structure in Galaxies, and uses the mid-infrared data of that survey to determine key parameters of the galaxies studied. From these data, important results are obtained on streaming and other non-circular motions in galaxies, on the distribution and rates of star formation, and on how correlations of these parameters and of the rotation curve shape with basic galaxy parameters yield clues on the evolutionary processes taking place in disk galaxies.
650
0
$a
Physics.
$3
179414
650
0
$a
Astronomy
$3
252518
650
0
$a
Astronomy
$x
Observations.
$3
560186
650
0
$a
Astrophysics.
$3
225419
650
2 4
$a
Astronomy, Observations and Techniques.
$3
376735
650
2 4
$a
Astrophysics and Astroparticles.
$3
376943
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/10.1007/978-3-319-26398-4
950
$a
Physics and Astronomy (Springer-11651)
筆 0 讀者評論
全部
電子館藏
館藏
1 筆 • 頁數 1 •
1
條碼號
館藏地
館藏流通類別
資料類型
索書號
使用類型
借閱狀態
預約狀態
備註欄
附件
000000121843
電子館藏
1圖書
電子書
EB QB4 E72 2016
一般使用(Normal)
在架
0
1 筆 • 頁數 1 •
1
多媒體
多媒體檔案
http://dx.doi.org/10.1007/978-3-319-26398-4
評論
新增評論
分享你的心得
Export
取書館別
處理中
...
變更密碼
登入