scholarly journals H_2O Megamasers: Accretion Disks, Jet Interaction, Outflows or Massive Star Formation?

2005 ◽  
Vol 295 (1-2) ◽  
pp. 107-116 ◽  
Author(s):  
C. Henkel ◽  
J. A. Braatz ◽  
A. Tarchi ◽  
A. B. Peck ◽  
N. M. Nagar ◽  
...  
2008 ◽  
Vol 4 (S259) ◽  
pp. 103-104 ◽  
Author(s):  
Rolf Kuiper ◽  
Mario Flock ◽  
Hubert Klahr

AbstractWe briefly overview our newly developed radiation transport module for MHD simulations and two actual applications. The method combines the advantage of the speed of the Flux-Limited Diffusion approximation and the high accuracy obtained in ray-tracing methods.


2009 ◽  
Vol 5 (H15) ◽  
pp. 801-801
Author(s):  
Stuart Lumsden ◽  
Melvin Hoare ◽  
Ben Davis ◽  

AbstractWe present the results of a Galaxy-wide survey for young massive stars still in the process of formation. Our data are consistent with a model in which the stars form through accretion disks with the overall Galactic star formation rate being 3 M⊙ per year.


2016 ◽  
Vol 225 (2) ◽  
pp. 21 ◽  
Author(s):  
Mihwa Jin ◽  
Jeong-Eun Lee ◽  
Kee-Tae Kim ◽  
Neal J. Evans II

2005 ◽  
Vol 1 (S227) ◽  
pp. 157-162 ◽  
Author(s):  
M. G. Burton ◽  
T. Hill ◽  
S. N. Longmore ◽  
C. R. Purcell ◽  
A. J. Walsh

2017 ◽  
Vol 13 (S332) ◽  
pp. 139-152
Author(s):  
Jonathan C. Tan

AbstractI review massive star formation in our Galaxy, focussing on initial conditions in Infrared Dark Clouds (IRDCs), including the search for massive pre-stellar cores (PSCs), and modeling of later stages of massive protostars, i.e., hot molecular cores (HMCs). I highlight how developments in astrochemistry, coupled with rapidly improving theoretical/computational and observational capabilities are helping to improve our understanding of the complex process of massive star formation.


Sign in / Sign up

Export Citation Format

Share Document