TY  -  
T1  - Galactic cold cores VIII. Filament formation and evolution : Filament properties in context with evolutionary models 
SN  -  /  
UR  - http://hdl.handle.net/10138/312765 
T3  -  
A1  - Rivera-Ingraham, A.; Ristorcelli, I.; Juvela, M.; Montillaud, J.; Men'shchikov, A.; Malinen, J.; Pelkonen, V. -M.; Marston, A.; Martin, P. G.; Pagani, L.; Paladini, R.; Paradis, D.; Ysard, N.; Ward-Thompson, D.; Bernard, J. -P.; Marshall, D. J.; Montier, L.; Toth, L. V. 
A2  -  
PB  -  
Y1  - 2017 
LA  - eng 
AB  - Context. The onset of star formation is intimately linked with the presence of massive unstable filamentary structures. These filaments are therefore key for theoretical models that aim to reproduce the observed characteristics of the star formation process in the Galaxy. Aims. As part of the filament study carried out by the Herschel Galactic Cold Cores Key Programme, here we study and discuss the filament properties presented in GCC VII (Paper I) in context with theoretical models of filament ... 
VO  -  
IS  -  
SP  -  
OP  -  
KW  - ISM: clouds; infrared: ISM; submillimeter: ISM; dust, extinction; stars: formation; STAR-FORMING FILAMENTS; MOLECULAR CLOUDS; GRAVITATIONAL COLLAPSE; FINITE SHEETS; HERSCHEL; TURBULENCE; GRAVITY; FRAGMENTATION; EMISSION; NEBULA; 115 Astronomy, Space science 
N1  -   
PP  -  
ER  -