東華大學圖書館 |

Language: English

Help

回圖書館首頁

手機版館藏查詢

Back

Switch To: Labeled | MARC Mode | ISBD

The earliest stages of massive clust...

Wang, Ke.

Linked to FindBook

Google Book

Amazon

博客來

The earliest stages of massive clustered star formation = fragmentation of infrared dark clouds /

Record Type:	Electronic resources : Monograph/item
Title/Author:	The earliest stages of massive clustered star formation/ by 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.
[NT 15003449]:	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.
Contained By:	Springer eBooks
Subject:	Stars - Formation. -
Online resource:	http://dx.doi.org/10.1007/978-3-662-44969-1
ISBN:	9783662449691 (electronic bk.)

The earliest stages of massive clustered star formation = fragmentation of infrared dark clouds /
Wang, Ke.

The earliest stages of massive clustered star formationfragmentation 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:

777194
Stars
--Formation.

LC Class. No.: QB806 / .W36 2015

Dewey Class. No.: 523.8

The earliest stages of massive clustered star formation = fragmentation of infrared dark clouds /
LDR:02173nmm a2200337 a 4500 001 1993925
003 DE-He213
005 20150721163052.0
006 m d
007 cr nn 008maaau
008 151019s2015 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 1057908
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 777194
650 1 4 $a Physics. $3 516296
650 2 4 $a Astronomy, Observations and Techniques. $3 1066822
650 2 4 $a Atmospheric Sciences. $3 1019179
650 2 4 $a Microwaves, RF and Optical Engineering. $3 893985
710 2 $a SpringerLink (Online service) $3 836513
773 0 $t Springer eBooks
830 0 $a Springer theses. $3 1314442
856 4 0 $u http://dx.doi.org/10.1007/978-3-662-44969-1
950 $a Physics and Astronomy (Springer-11651)