Determination of the W-182/W-184 ratio to a precision of +/- 5 ppm (2 sigma) is desirable for constraining the timing of core formation and other early planetary differentiation processes. However, WO3- analysis by negative thermal ionization mass spectrometry normally results in a residual correlation between the instrumental-mass-fractionation-corrected (182)w/(184)w and W-183/W-184 ratios that is attributed to mass-dependent variability of 0 isotopes over the course of an analysis and between different analyses. A second-order correction using the W-183/W-184 ratio relies on the assumption that this ratio is constant in nature. This may prove invalid, as has already been realized for other isotope systems. The present study utilizes simu...
The short-lived radionuclide, 182Hf (t1/2 = 8.9 million years) decays to 182W (natural abundance 26%...
Excesses and deficiencies in 182W in meteorites and lunar samples relative to the terrestrial 182W a...
Abstract—The rates of accretion and core formation of the Earth and other inner solar system objects...
Determination of the W-182/W-184 ratio to a precision of +/- 5 ppm (2 sigma) is desirable for constr...
We present a double-spike technique for precise determination of mass-dependent fractionation of tun...
Mass-dependent isotope fractionation of tungsten (W) isotopes has not received much attention until ...
We present new high precision Os isotope data obtained by solution-mode MC-ICP-MS for 4 different Os...
Optical isotope shifts of the five stable isotopes of tungsten ( 180W, 182W, 183W, 184W and 186 W) a...
An obstacle for establishing the chronology of iron meteorite formation using 182Hf-182W systematics...
Osmium stable isotopes provide a new, potentially powerful tool with which to investigate a diverse ...
From the line 5 642 Å (d4 5s2 D1 — d4 sp 7 F°0), the relative isotope shift of the four abundant iso...
Tungsten isotope compositions of magmatic iron meteorites yield ages of differentiation that are wit...
The stable isotope ratio of W is a new tracer in oceanographic studies and a new proxy in paleoceano...
High-precision tungsten (W-182/(184)w) isotope measurements on well-characterised mafic and felsic s...
International audienceLifetimes of yrast states in the rare-earth midshell isotopes W176,178,180 hav...
The short-lived radionuclide, 182Hf (t1/2 = 8.9 million years) decays to 182W (natural abundance 26%...
Excesses and deficiencies in 182W in meteorites and lunar samples relative to the terrestrial 182W a...
Abstract—The rates of accretion and core formation of the Earth and other inner solar system objects...
Determination of the W-182/W-184 ratio to a precision of +/- 5 ppm (2 sigma) is desirable for constr...
We present a double-spike technique for precise determination of mass-dependent fractionation of tun...
Mass-dependent isotope fractionation of tungsten (W) isotopes has not received much attention until ...
We present new high precision Os isotope data obtained by solution-mode MC-ICP-MS for 4 different Os...
Optical isotope shifts of the five stable isotopes of tungsten ( 180W, 182W, 183W, 184W and 186 W) a...
An obstacle for establishing the chronology of iron meteorite formation using 182Hf-182W systematics...
Osmium stable isotopes provide a new, potentially powerful tool with which to investigate a diverse ...
From the line 5 642 Å (d4 5s2 D1 — d4 sp 7 F°0), the relative isotope shift of the four abundant iso...
Tungsten isotope compositions of magmatic iron meteorites yield ages of differentiation that are wit...
The stable isotope ratio of W is a new tracer in oceanographic studies and a new proxy in paleoceano...
High-precision tungsten (W-182/(184)w) isotope measurements on well-characterised mafic and felsic s...
International audienceLifetimes of yrast states in the rare-earth midshell isotopes W176,178,180 hav...
The short-lived radionuclide, 182Hf (t1/2 = 8.9 million years) decays to 182W (natural abundance 26%...
Excesses and deficiencies in 182W in meteorites and lunar samples relative to the terrestrial 182W a...
Abstract—The rates of accretion and core formation of the Earth and other inner solar system objects...