ErIII-Cored Complexes Based on Dendritic PtII–Porphyrin Ligands: Synthesis, Near-IR Emission Enhancement, and Photophysical Studies

2007 ◽  
Vol 17 (3) ◽  
pp. 413-424 ◽  
Author(s):  
J. B. Oh ◽  
M.-K. Nah ◽  
Y. H. Kim ◽  
M. S. Kang ◽  
J.-W. Ka ◽  
...  
2011 ◽  
Vol 24 (6) ◽  
pp. 887-895 ◽  
Author(s):  
Miriam Uemi ◽  
Graziella E. Ronsein ◽  
Fernanda M. Prado ◽  
Flávia D. Motta ◽  
Sayuri Miyamoto ◽  
...  

2009 ◽  
Vol 473 (1-2) ◽  
pp. 500-504 ◽  
Author(s):  
M. Alejandrina Martínez Gámez ◽  
A.V. Kir’yanov ◽  
J.L. Lucio M. ◽  
C. Wiechers ◽  
G.A. Kumar
Keyword(s):  
Near Ir ◽  

Author(s):  
Vicente Vargas ◽  
Anastasiya Sedova ◽  
Jesús Uriel Balderas ◽  
S. Carmona-Tellez ◽  
Iván Merlin ◽  
...  

2015 ◽  
Vol 51 (12) ◽  
pp. 2372-2375 ◽  
Author(s):  
Zhiyu Liao ◽  
Manuel Tropiano ◽  
Konstantins Mantulnikovs ◽  
Stephen Faulkner ◽  
Tom Vosch ◽  
...  

NIR imaging of lanthanide-coated silica particles where the photons used to generate the image unambiguously can be assigned to arise from lanthanide centred emission.


1993 ◽  
Vol 155 ◽  
pp. 386-386
Author(s):  
J.P. Harrington ◽  
K.J. Borkowski ◽  
W.P. Blair ◽  
J. Bregman

High-resolution images in [O III] λ5007 of the hydrogen-poor knots of Abell 30 reveal comet-like structures which may be indicative of interaction with the stellar wind. In the near IR, new, higher-resolution, K-band images show an equatorial ring of hot dust that corresponds closely to optical knots 2 and 4 of Jacoby and Ford, while their polar knots 1 and 3 show no comparable IR emission. Both the thermal IR emission and the heavy internal extinction of the central star demands an extremely dusty ejecta. Greenstein showed that the UV extinction curve is fit by amorphous carbon. Our comprehensive dust models consider both the UV extinction and the IR emission from a population of carbon grains. The thermal emission from larger grains produces the far IR emission, while the stochastic heating of very small grains to high temperatures is essential to explain the near IR flux. We are able to reproduce the shape of the near IR spectrum with an a−3.0 distribution of grain radii which extends down to a minimum grain radius of 8 Å.


2004 ◽  
Vol 30 (2) ◽  
pp. 191-205 ◽  
Author(s):  
Munenori Ryo ◽  
Yuji Wada ◽  
Tatsuya Okubo ◽  
Shozo Yanagida

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