Scientific role of ACA for low-mass star-formation study

Author(s):  
Shigehisa Takakuwa ◽  
Daisuke Iono ◽  
Baltasar Vila-Vilaro ◽  
Tomohiko Sekiguchi ◽  
Ryohei Kawabe
Keyword(s):  
2013 ◽  
Vol 554 ◽  
pp. A48 ◽  
Author(s):  
V. M. Rivilla ◽  
J. Martín-Pintado ◽  
I. Jiménez-Serra ◽  
A. Rodríguez-Franco

2007 ◽  
Vol 313 (1-3) ◽  
pp. 169-173 ◽  
Author(s):  
Shigehisa Takakuwa ◽  
Daisuke Iono ◽  
Baltasar Vila-Vilaro ◽  
Tomohiko Sekiguchi ◽  
Ryohei Kawabe
Keyword(s):  

1998 ◽  
Vol 508 (1) ◽  
pp. 347-369 ◽  
Author(s):  
K. L. Luhman ◽  
G. H. Rieke ◽  
C. J. Lada ◽  
E. A. Lada

2013 ◽  
Vol 557 ◽  
pp. A35 ◽  
Author(s):  
Eduard I. Vorobyov ◽  
Isabelle Baraffe ◽  
Tim Harries ◽  
Gilles Chabrier

2006 ◽  
Vol 2 (S237) ◽  
pp. 124-127
Author(s):  
L. Viktor Tóth ◽  
Zoltán T. Kiss

AbstractOur goal is to evaluate the role of triggering effects on the star formation and early stellar evolution by presenting a statistically large sample of cloud and low-mass YSO data. We conducted large area surveys (ranging from 400 square-degree to 10800 square-degree) in optical, NIR and FIR. The distribution of the ISM and low-mass YSOs were surveyed. A relative excess was found statistically in the number of dense and cold core bearing clouds and low mass YSOs in the direction of the FIR loop shells indicating a possible excess in their formation.


2012 ◽  
Vol 747 (1) ◽  
pp. 22 ◽  
Author(s):  
Charles E. Hansen ◽  
Richard I. Klein ◽  
Christopher F. McKee ◽  
Robert T. Fisher

2010 ◽  
Vol 6 (S270) ◽  
pp. 103-106
Author(s):  
R. Rao ◽  
J.-M. Girart ◽  
D. P. Marrone

AbstractThere have been a number of theoretical and computational models which state that magnetic fields play an important role in the process of star formation. Competing theories instead postulate that it is turbulence which is dominant and magnetic fields are weak. The recent installation of a polarimetry system at the Submillimeter Array (SMA) has enabled us to conduct observations that could potentially distinguish between the two theories. Some of the nearby low mass star forming regions show hour-glass shaped magnetic field structures that are consistent with theoretical models in which the magnetic field plays a dominant role. However, there are other similar regions where no significant polarization is detected. Future polarimetry observations made by the Submillimeter Array should be able to increase the sample of observed regions. These measurements will allow us to address observationally the important question of the role of magnetic fields and/or turbulence in the process of star formation.


Author(s):  
T. W. Hartquist ◽  
J. E. Dyson
Keyword(s):  

1982 ◽  
Vol 257 ◽  
pp. 620 ◽  
Author(s):  
P. C. Myers
Keyword(s):  

1986 ◽  
Vol 302 ◽  
pp. 352 ◽  
Author(s):  
J. A. Graham
Keyword(s):  

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