Iron meteorites and their weathering products: high-velocity-resolution M�ssbauer spectroscopy of the iron-bearing minerals

2016 ◽  
Keyword(s):  
High Velocity ◽  
Iron Meteorites ◽  
High Velocity Resolution ◽  
Ssbauer Spectroscopy ◽  
Iron Bearing

Iron meteorites and their weathering products: high velocity resolution Mössbauer spectroscopy of the iron-bearing minerals

2016 ◽  
Vol 28 (3) ◽  
pp. 601-610 ◽  
Author(s):  
Mikhail V. Goryunov ◽  
Grigoriy A. Yakovlev ◽  
Andrei V. Chukin ◽  
Victor I. Grokhovsky ◽  
Vladimir A. Semionkin ◽  
...  
Keyword(s):  
Mössbauer Spectroscopy ◽  
High Velocity ◽  
Mossbauer Spectroscopy ◽  
Iron Meteorites ◽  
High Velocity Resolution ◽  
Mößbauer Spectroscopy ◽  
Iron Bearing

Mossbauer spectroscopy with high velocity resolution in the study of iron-bearing minerals in meteorites

2009 ◽  
Vol 21 (1) ◽  
pp. 51-63 ◽  
Author(s):  
Victor I. Grokhovsky ◽  
Michael I. Oshtrakh ◽  
Evgeniya V. Petrova ◽  
Mikhail Yu. Larionov ◽  
Kseniya A. Uymina ◽  
...  
Keyword(s):  
Mössbauer Spectroscopy ◽  
High Velocity ◽  
Mossbauer Spectroscopy ◽  
High Velocity Resolution ◽  
Mößbauer Spectroscopy ◽  
Iron Bearing

scholarly journals Mössbauer spectroscopy with a high velocity resolution applied for the study of meteoritic iron-bearing minerals

2013 ◽  
Vol 1044 ◽  
pp. 268-278 ◽  
Author(s):  
M.I. Oshtrakh ◽  
V.I. Grokhovsky ◽  
E.V. Petrova ◽  
M.Yu. Larionov ◽  
M.V. Goryunov ◽  
...  
Keyword(s):  
Mössbauer Spectroscopy ◽  
High Velocity ◽  
Mossbauer Spectroscopy ◽  
High Velocity Resolution ◽  
Mößbauer Spectroscopy ◽  
Meteoritic Iron ◽  
Iron Bearing

scholarly journals 13CO(J = 1-0) Observations of the Orion Molecular Cloud

1987 ◽  
Vol 115 ◽  
pp. 149-150
Author(s):  
K. Sugitani ◽  
Y. Fukui
Keyword(s):  
Millimeter Wave ◽  
High Velocity ◽  
Molecular Cloud ◽  
High Velocity Resolution ◽  
H Ii Region ◽  
Co Emission

We present new 13CO(J = 1-0) measurements of the Orion molecular cloud. The data were taken with the 4-m millimeter-wave telescope of Nagoya University with a beamwidth of 2.7′. The high velocity resolution of 0.1 km s−1 employed has revealed significant details of the 13CO emission toward the H II region.

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