Titlebook: Dense Molecular Gas around Protostars and in Galactic Nuclei; European Workshop on W.A. Baan,Y. Hagiwara,H.J. Langevelde Book 2005 Springer

fiction

邊緣帶來(lái)墨水

Endoscope

emission

Nicholas Roussopoulos,Wilfrid Utzn pressure should reverse the infall thus preventing further growth of the stellar mass. After illustrating the two models proposed to solve this problem (“accretion” and “coalescence”), we review the observational evidence pro/contra such models, focusing on the kinematics of the molecular gas wher

PRO

Nicholas Roussopoulos,Wilfrid Utz from the Puschino radio telescope. The drift velocities of the masers and the velocity and location of a new maser region add depth to the model of two colliding CO clouds triggering collapse. Some H.O masers appear to originate directly from this shock front. The brightest maser appears typical of

NATAL

https://doi.org/10.1007/978-3-030-73758-0ervational method favours different regimes of scale size, density and other physical conditions. The available techniques and their ranges of applicability are briefly described and the current status of observations is reviewed, with particular emphasis on high-resolution observations of star-form

inchoate

MELD

錫箔紙

古董