Preliminary results on the LC-separation of non-steroidal anti-inflammatory agents in conventional and narrow-bore RP setups applying columns with different internal diameters

1995 ◽  
Vol 9 (6) ◽  
pp. 261-262 ◽  
Author(s):  
W. R. G. Baeyens ◽  
G. Van der Weken ◽  
A. Van Overbeke ◽  
Z. D. Zhang
2018 ◽  
Vol 14 (2) ◽  
pp. 336-344 ◽  
Author(s):  
Mario Adan Moreno-Eutimio ◽  
Lorena Espinosa-Monroy ◽  
Tania Orozco-Amaro ◽  
Yessica Torres-Ramos ◽  
Araceli Montoya-Estrada ◽  
...  

2018 ◽  
Vol 64 (8) ◽  
pp. 78 ◽  
Author(s):  
Federico Scotti ◽  
Sem Decani ◽  
Andrea Sardella ◽  
Marcello Iriti ◽  
Elena Maria Varoni ◽  
...  

2017 ◽  
Vol 62 (12) ◽  
pp. 3468-3478 ◽  
Author(s):  
Deepesh Sharma ◽  
Aparna Jakkampudi ◽  
Ratnakar Reddy ◽  
Panyala Balakumar Reddy ◽  
Aasish Patil ◽  
...  

Author(s):  
Mario Adan Moreno-Eutimio ◽  
Lorena Espinosa-Monroy ◽  
Tania Orozco-Amaro ◽  
Yessica Torres-Ramos ◽  
Araceli Montoya-Estrada ◽  
...  

1999 ◽  
Vol 173 ◽  
pp. 185-188
Author(s):  
Gy. Szabó ◽  
K. Sárneczky ◽  
L.L. Kiss

AbstractA widely used tool in studying quasi-monoperiodic processes is the O–C diagram. This paper deals with the application of this diagram in minor planet studies. The main difference between our approach and the classical O–C diagram is that we transform the epoch (=time) dependence into the geocentric longitude domain. We outline a rotation modelling using this modified O–C and illustrate the abilities with detailed error analysis. The primary assumption, that the monotonity and the shape of this diagram is (almost) independent of the geometry of the asteroids is discussed and tested. The monotonity enables an unambiguous distinction between the prograde and retrograde rotation, thus the four-fold (or in some cases the two-fold) ambiguities can be avoided. This turned out to be the main advantage of the O–C examination. As an extension to the theoretical work, we present some preliminary results on 1727 Mette based on new CCD observations.


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