Linearly Polarized Emission from Colloidal Semiconductor Quantum Rods

Science ◽  
2001 ◽  
Vol 292 (5524) ◽  
pp. 2060-2063 ◽  
Author(s):  
J. Hu
2008 ◽  
Vol 53 (9(5)) ◽  
pp. 2782-2786
Author(s):  
Yu. G. Kusrayev ◽  
A. V. Koudinov ◽  
N. S. Averkiev ◽  
D. Wolverson ◽  
J. J. Davies ◽  
...  

Nano Letters ◽  
2020 ◽  
Vol 20 (6) ◽  
pp. 4204-4210 ◽  
Author(s):  
Huilin He ◽  
Jianxun Liu ◽  
Ke Li ◽  
Zhen Yin ◽  
Jiawei Wang ◽  
...  

2019 ◽  
Vol 99 (15) ◽  
Author(s):  
A. Mitioglu ◽  
S. Anghel ◽  
M. V. Ballottin ◽  
K. Sushkevich ◽  
L. Kulyuk ◽  
...  

2017 ◽  
Vol 25 (4) ◽  
pp. 3737 ◽  
Author(s):  
Dong-Myoung Lee ◽  
You-Jin Lee ◽  
Jae-Hoon Kim ◽  
Chang-Jae Yu

2013 ◽  
Vol 21 (25) ◽  
pp. 31591 ◽  
Author(s):  
Sebastian Knitter ◽  
Michael Kues ◽  
Michael Haidl ◽  
Carsten Fallnich

2020 ◽  
Vol 28 (23) ◽  
pp. 34337
Author(s):  
Kaifei Tang ◽  
Wenbin Liao ◽  
Ke Li ◽  
Bingxuan Li ◽  
Weidong Chen ◽  
...  

1983 ◽  
Vol 101 ◽  
pp. 343-346
Author(s):  
C. J. Salter ◽  
F. Mantovani ◽  
P. Tomasi

High resolution maps of the Galactic radio source CTB80 at three different frequencies are presented. A new interpretation in terms of a cosmic collision between two SNRs of different age is suggested.CTB80 is one of the most mystifying Galactic Objects yet discovered and has recently attracted considerable attention from X-ray, optical and radio astronomers (see for example: Becker et al. (1981), Angerhofer et al. (1980, 1981), Velusamy et al. (1976), van den Bergh (1980).The present observations of the radio continuum emission of the extended feature at 408 MHz, 1720 MHz and 4750 MHz and the linearly polarized emission at 1720 MHz and 4750 MHz (Figs 1,2,3) throw new light on the morphological, spectral and polarization properties of the whole source.


1990 ◽  
Vol 140 ◽  
pp. 219-222
Author(s):  
E. Hummel ◽  
M. Dahlem

We observed the linearly polarized emission of the edge-on galaxies NGC891 and NGC4631 in order to determine the magnetic field structure.


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