ICP-MS applied to isotope abundance ratio measurements: Performance study and development of a method for combining uncertainty contributions from measurement correction factors

2007 ◽  
pp. 257-269 ◽  
Author(s):  
Christophe R. Quetel ◽  
Thomas Prohaska ◽  
Simon M. Nelms ◽  
Jurgen Diemer ◽  
Philip D. P. Taylor
2011 ◽  
Vol 7 (S283) ◽  
pp. 502-503
Author(s):  
Richard A. Shaw ◽  
Ting-Hui Lee ◽  
Letizia Stanghellini ◽  
James E. Davies ◽  
D. Anibal García-Hernández ◽  
...  

AbstractWe determine elemental abundances of He, N, O, Ne, S, and Ar in Magellanic Cloud planetary nebulae (PNe) using direct methods and a large set of observed ions, minimizing the need for ionization correction factors. In contrast to prior studies, we find a clear separation between Type I and non-Type I PNe in these low-metallicity environments, and no evidence that the O-N nucleosynthesis cycle is active in low-mass progenitors. We find that the S/O abundance ratio is anomalously low compared to H ii regions, confirming the “sulfur anomaly” found for Galactic PNe. We also found that Ne/O is elevated in some cases, raising the possibility that Ne yields in low-mass AGB stars may be enhanced at low metallicity.


2019 ◽  
Vol 34 (10) ◽  
pp. 2094-2104 ◽  
Author(s):  
Skyler W. Smith ◽  
Nicole Hanks ◽  
Patricia A. Creed ◽  
Kasey Kovalcik ◽  
Robert A. Wilson ◽  
...  

Rare earth elements (REE) can produce M2+ ions in ICP-MS and 150Nd2+, 150Sm2+, and 156Gd2+ can produce false positives on 75As and 78Se.


2011 ◽  
Vol 7 (S283) ◽  
pp. 488-489
Author(s):  
Mónica Rodríguez ◽  
Gloria Delgado-Inglada

AbstractWe derive the chlorine abundances in a sample of nearby planetary nebulae (PNe) and H II regions that have some of the best available spectra. We use a nearly homogeneous procedure to derive the abundance in each object and find that the Cl/H abundance ratio shows similar values in H II regions and PNe. This supports our previous interpretation that the underabundance we found for oxygen in the H II regions is due to the depletion of their oxygen atoms into organic refractory dust components. For other elements, the bias introduced by ionization correction factors in their derived abundances can be very important, as we illustrate here for sulfur using photoionization models. Even for low-ionization PNe, the derived sulfur abundances can be lower than the real ones by up to 0.3 dex, and the differences found with the abundances derived for H II regions that have similar S/H can reach 0.4 dex.


1995 ◽  
Vol 439 ◽  
pp. 1021 ◽  
Author(s):  
Marvin Kleine ◽  
Susan Wyckoff ◽  
Peter A. Wehinger ◽  
Bruce A. Peterson

2004 ◽  
Vol 19 (2) ◽  
pp. 227 ◽  
Author(s):  
G. Fortunato ◽  
K. Mumic ◽  
S. Wunderli ◽  
L. Pillonel ◽  
J. O. Bosset ◽  
...  

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