RADIO JETS AND DISKS IN THE INTERMEDIATE-MASS STAR-FORMING REGION NGC2071IR

2009 ◽  
Vol 706 (1) ◽  
pp. 244-251 ◽  
Author(s):  
M. A. Trinidad ◽  
T. Rodríguez ◽  
L. F. Rodríguez
2009 ◽  
Vol 691 (1) ◽  
pp. 332-341 ◽  
Author(s):  
Luis A. Zapata ◽  
Karl Menten ◽  
Mark Reid ◽  
Henrik Beuther

2016 ◽  
Vol 822 (2) ◽  
pp. 79 ◽  
Author(s):  
Mária Kun ◽  
Attila Moór ◽  
Elza Szegedi-Elek ◽  
Bo Reipurth

2010 ◽  
Vol 140 (2) ◽  
pp. 462-479 ◽  
Author(s):  
K. Arvidsson ◽  
C. R. Kerton ◽  
M. J. Alexander ◽  
H. A. Kobulnicky ◽  
B. Uzpen

2006 ◽  
Vol 2 (S237) ◽  
pp. 406-406 ◽  
Author(s):  
Joanne Dawson ◽  
A. Kawamura ◽  
N. Mizuno ◽  
T. Onishi ◽  
Y. Fukui

AbstractTheory predicts the triggered formation of molecular clouds stars through the fragmentation and collapse of swept-up ambient gas. Yet the majority of Galactic HI shells show no more than a scattering of small molecular clouds. The Carina Flare supershell (Fukui et al. 1999) is a rare example of an HI shell with a striking molecular component. Here we present the large-scale morphology of the molecular and atomic gas and the location of YSO candidates. A detailed look at two molecular clumps in the shell walls reveals active, intermediate mass star forming regions at various stages of early evolution.


2014 ◽  
Vol 442 (1) ◽  
pp. 148-159 ◽  
Author(s):  
J. M. Torrelles ◽  
S. Curiel ◽  
R. Estalella ◽  
G. Anglada ◽  
J. F. Gómez ◽  
...  

2014 ◽  
Vol 784 (2) ◽  
pp. 111 ◽  
Author(s):  
Michael J. Lundquist ◽  
Henry A. Kobulnicky ◽  
Michael J. Alexander ◽  
Charles R. Kerton ◽  
Kim Arvidsson

Author(s):  
M. Solimano ◽  
J. González-López ◽  
L. F. Barrientos ◽  
M. Aravena ◽  
S. López ◽  
...  

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