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The earliest stages of massive clust...

Wang, Ke.

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

紀錄類型:	書目-電子資源 : Monograph/item
正題名/作者:	The earliest stages of massive clustered star formation/ by Ke Wang.
其他題名:	fragmentation of infrared dark clouds /
作者:	Wang, Ke.
出版者:	Berlin, Heidelberg :Springer Berlin Heidelberg : : 2015.,
面頁冊數:	xx, 145 p. :ill. (some col.), digital ;24 cm.
內容註:	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
標題:	Stars - Formation. -
電子資源:	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

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