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Some strong reflections about 3 to 5 m thick were observed at depths of 25-60 metres below the sea floor using deep-towed, 5 kHz subbottom profiler data in the Turkish shelf and upper slope of the Ea...
High resolution spectroscopy of planet bearing stars      spectroscopy  planet bearing stars       font style='font-size:12px;'> 2009/7/1
High resolution spectroscopy of planet bearing stars
A high resolution scanning fabry-perot for OSIRIS     fabry-perot  scanning  OSIRIS       font style='font-size:12px;'> 2009/7/1
A high resolution scanning fabry-perot for OSIRIS。
High resolution spectra of novae and the quadratic zeeman effect      High resolution spectra  novae       font style='font-size:12px;'> 2009/6/25
High resolution spectra of novae and the quadratic zeeman effect。
High resolution oh maser survey in star forming regions     maser survey  star forming regions       font style='font-size:12px;'> 2009/6/25
High resolution oh maser survey in star forming regions。
Stromgren Photometry and High Resolution Spectroscopy of Very Metal-Poor Stars
Stellar Tools for High Resolution Population Synthesis。
Using high resolution data to investigate the variability Of gg carinae system。
First High Resolution Simulations of the Local Bubble     Local Bubble  First High Resolution Simulations       font style='font-size:12px;'> 2009/6/16
First High Resolution Simulations of the Local Bubble。
High Resolution X-Ray Observations of Pulsar Winds     X-Ray Observations  Pulsar Winds       font style='font-size:12px;'> 2009/6/16
High Resolution X-Ray Observations of Pulsar Winds。
High Resolution X-Ray Observations of Pulsar Winds     X-Ray Observations  Pulsar Winds       font style='font-size:12px;'> 2009/6/16
High Resolution X-Ray Observations of Pulsar Winds。
High Resolution Spectra of Stellar Winds in Very Young Massive Stars
An updated version of the nested-grid GEOS-Chem model is developed allowing for higher horizontal (0.5°×0.667°) resolution as compared to global models. CO transport over a heavily polluted region, th...
The need for very high resolution spectroscopy for the study of hot subdwarfs。
A High Resolution H I Study of the ISM Local to Galactic Wolf-rayet Stars

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