Language:
English
繁體中文
Help
圖資館首頁
Login
Back
Switch To:
Labeled
|
MARC Mode
|
ISBD
The earliest stages of massive clust...
~
SpringerLink (Online service)
The earliest stages of massive clustered star formationfragmentation of infrared dark clouds /
Record Type:
Electronic resources : Monograph/item
Title/Author:
The earliest stages of massive clustered star formationby Ke Wang.
Reminder of title:
fragmentation of infrared dark clouds /
Author:
Wang, Ke.
Published:
Berlin, Heidelberg :Springer Berlin Heidelberg :2015.
Description:
xx, 145 p. :ill. (some col.), digital ;24 cm.
Contained By:
Springer eBooks
Subject:
StarsFormation.
Online resource:
http://dx.doi.org/10.1007/978-3-662-44969-1
ISBN:
9783662449691 (electronic bk.)
The earliest stages of massive clustered star formationfragmentation of infrared dark clouds /
Wang, Ke.
The earliest stages of massive clustered star formation
fragmentation of infrared dark clouds /[electronic resource] :by Ke Wang. - Berlin, Heidelberg :Springer Berlin Heidelberg :2015. - xx, 145 p. :ill. (some col.), digital ;24 cm. - Springer theses,2190-5053. - Springer theses..
Scientific background -- An Infrared Point Source Survey -- The Dragon Nebula G28.34+0.06 -- The Snake Nebula G11.11-0.12 -- The Infrared Dark Cloud G30.88+0.13 -- A New Evolutionary Picture.
This thesis presents an in-depth, high-resolution observational study on the very beginning of the formation process: the fragmentation of dense molecular clouds known as infrared dark clouds (IRDCs). Using the Submillimeter Array (SMA) and Very Large Array (VLA) radio interferometers, the author has discovered a common picture of hierarchical fragmentation that challenges some of the leading theoretical models and suggests a new, observation-driven understanding of how massive star formation in clustered environments may begin: it is initiated by the hierarchical fragmentation of a dense filament from 10 pc down to 0.01 pc, and the stellar mass buildup is simultaneously fed by hierarchical accretion at similar scales. The new scenario points out the importance of turbulence and filamentary structure, which are now receiving increasing attention and further tests from both observers and theorists.
ISBN: 9783662449691 (electronic bk.)
Standard No.: 10.1007/978-3-662-44969-1doiSubjects--Topical Terms:
274157
Stars
--Formation.
LC Class. No.: QB806 / .W36 2015
Dewey Class. No.: 523.8
The earliest stages of massive clustered star formationfragmentation of infrared dark clouds /
LDR
:02173nmm a2200337 a 4500
001
460911
003
DE-He213
005
20150721163052.0
006
m d
007
cr nn 008maaau
008
151110s2015 gw s 0 eng d
020
$a
9783662449691 (electronic bk.)
020
$a
9783662449684 (paper)
024
7
$a
10.1007/978-3-662-44969-1
$2
doi
035
$a
978-3-662-44969-1
040
$a
GP
$c
GP
041
0
$a
eng
050
4
$a
QB806
$b
.W36 2015
072
7
$a
PG
$2
bicssc
072
7
$a
SCI004000
$2
bisacsh
072
7
$a
NAT033000
$2
bisacsh
082
0 4
$a
523.8
$2
23
090
$a
QB806
$b
.W246 2015
100
1
$a
Wang, Ke.
$3
712686
245
1 4
$a
The earliest stages of massive clustered star formation
$h
[electronic resource] :
$b
fragmentation of infrared dark clouds /
$c
by Ke Wang.
260
$a
Berlin, Heidelberg :
$b
Springer Berlin Heidelberg :
$b
Imprint: Springer,
$c
2015.
300
$a
xx, 145 p. :
$b
ill. (some col.), digital ;
$c
24 cm.
490
1
$a
Springer theses,
$x
2190-5053
505
0
$a
Scientific background -- An Infrared Point Source Survey -- The Dragon Nebula G28.34+0.06 -- The Snake Nebula G11.11-0.12 -- The Infrared Dark Cloud G30.88+0.13 -- A New Evolutionary Picture.
520
$a
This thesis presents an in-depth, high-resolution observational study on the very beginning of the formation process: the fragmentation of dense molecular clouds known as infrared dark clouds (IRDCs). Using the Submillimeter Array (SMA) and Very Large Array (VLA) radio interferometers, the author has discovered a common picture of hierarchical fragmentation that challenges some of the leading theoretical models and suggests a new, observation-driven understanding of how massive star formation in clustered environments may begin: it is initiated by the hierarchical fragmentation of a dense filament from 10 pc down to 0.01 pc, and the stellar mass buildup is simultaneously fed by hierarchical accretion at similar scales. The new scenario points out the importance of turbulence and filamentary structure, which are now receiving increasing attention and further tests from both observers and theorists.
650
0
$a
Stars
$x
Formation.
$3
274157
650
1 4
$a
Physics.
$3
179414
650
2 4
$a
Astronomy, Observations and Techniques.
$3
376735
650
2 4
$a
Atmospheric Sciences.
$3
264356
650
2 4
$a
Microwaves, RF and Optical Engineering.
$3
274186
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/10.1007/978-3-662-44969-1
950
$a
Physics and Astronomy (Springer-11651)
based on 0 review(s)
ALL
電子館藏
Items
1 records • Pages 1 •
1
Inventory Number
Location Name
Item Class
Material type
Call number
Usage Class
Loan Status
No. of reservations
Opac note
Attachments
000000110418
電子館藏
1圖書
電子書
EB QB806 W246 2015
一般使用(Normal)
On shelf
0
1 records • Pages 1 •
1
Multimedia
Multimedia file
http://dx.doi.org/10.1007/978-3-662-44969-1
Reviews
Add a review
and share your thoughts with other readers
Export
pickup library
Processing
...
Change password
Login