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The understanding of evolution of solar system has been recently entered a phase of major change with the results of new astronomical observation, several primitive extraterrestrial samples includi...
The chemistry of the early Universe is a fascinating field of study. Even in the absence of any elements heavier than lithium, a surprising degree of chemical complexity proves to be possible, giving ...
Until now, axisymmetric, alpha-disc models have been adopted for calculations of the chemical composition of protoplanetary discs. While this approach is reasonable for many discs, it is not appropria...
We apply the method of Burnett & Binney (2010) for the determination of stellar distances and parameters to the internal catalogue of the Radial Velocity Experiment (Steinmetz et al. 2006). Subsamples...
A review of non-local, deep transport mechanisms in the atmosphere of Earth provides a good foundation for examining whether similar mechanisms are operating in the atmospheres of Mars and Titan. On E...
We present the comparison of the three most important ice constituents (water, CO and CO2) in the envelopes of massive Young Stellar Objects (YSOs), in environments of differentmetallicities:the Gala...
Chemistry in Evaporating Ices: Unexplored Territory      astrochemistry – ISM  molecules  ISM  clouds       font style='font-size:12px;'> 2010/11/15
We suggest that three–body chemistry may occur in warm high density gas evaporating in transient co–desorption events on interstellar ices. Using a highly idealised computational model we explore the ...
The astrochemistry of the HnO+ (n=1..3) ions is important as the main gas-phase formation route for water, and as tracer of the interstellar ionization rate by cosmic rays and other processes. While i...
We present results from a model of the chemical evolution of protoplanetary disks. In our models we directly calculate the changing propagation and penetration of a high energy radiation field with Ly...
Gas Heating, Chemistry, and Infrared Spectra in Intermediate-Aged Disks Around Low Mass Stars。
Physics and chemistry of planetary nebulae with ISO-SWS     Physics  chemistry  planetary nebulae  ISO-SWS       font style='font-size:12px;'> 2009/6/11
Physics and chemistry of planetary nebulae with ISO-SWS。
The chemistry of stellar Jets     stellar Jets  chemistry       font style='font-size:12px;'> 2009/6/10
The chemistry of stellar Jets。
The Study of Interstellar Chemistry Through Mid-Infrared Spectroscopy。
We have constructed two gas-phase models to study the chemistry of circumstellar envelope surrounding the carbon-rich variable star IRAS 15194–5115. The network used consists of 3893 reactions invol...
We have constructed two gas-phase models to study the chemistry of circumstellar envelope surrounding the carbon-rich variable star IRAS 15194–5115. The network used consists of 3893 reactions involvi...

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