narrow spectral line
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Author(s):  
Bernd Sumpf ◽  
Lara Sophie Theurer ◽  
Martin Maiwald ◽  
André Müller ◽  
Andre Maaßdorf ◽  
...  

ACS Nano ◽  
2020 ◽  
Vol 14 (6) ◽  
pp. 6906-6911
Author(s):  
Jie Bai ◽  
Yuefei Cai ◽  
Peng Feng ◽  
Peter Fletcher ◽  
Chenqi Zhu ◽  
...  

2016 ◽  
Vol 122 (8) ◽  
Author(s):  
C. Yang ◽  
Y. L. Ju ◽  
B. Q. Yao ◽  
T. Y. Dai ◽  
X. M. Duan ◽  
...  

2015 ◽  
Vol 54 (17) ◽  
pp. 5420 ◽  
Author(s):  
Bo Liu ◽  
Xin Tong ◽  
Chenyang Jiang ◽  
Daniel R. Brown ◽  
Lee Robertson

2012 ◽  
Vol 8 (S287) ◽  
pp. 69-73
Author(s):  
Gabriele Surcis ◽  
Wouter H. T. Vlemmings ◽  
Huib J. van Langevelde ◽  
Busaba Hutawarakorn Kramer

AbstractThe bright and narrow spectral line emission of masers is ideal for measuring the Zeeman-splitting as well as for determining the orientation of magnetic fields in 3-dimensions around massive protostars. Recently, polarization observations at milliarcsecond resolution of 6.7-GHz CH3OH masers have uniquely been able to resolve the morphology of magnetic fields close to massive protostars. The observations reveal that the magnetic fields are along outflows and/or on the surfaces of circumstellar tori. Here we present three different examples selected from a total number of 7 massive star-forming regions that were investigated at 6.7-GHz with the EVN in the last years.


Author(s):  
D.V. Kuksenkov ◽  
E.M. Kosik Williams ◽  
A.S. Bauco ◽  
R.A. Hoyt ◽  
S. Li ◽  
...  

2003 ◽  
Vol 76 (6) ◽  
pp. 633-637 ◽  
Author(s):  
S. Civiš ◽  
P. Kubát ◽  
Z. Zelinger ◽  
V. Horká ◽  
A.N. Imenkov ◽  
...  

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