期刊论文详细信息
Journal of astrophysics and astronomy
MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center
M. S. Dimitrijević45  D. Jevremović3  Lj. M. Ignjatović4  A. A. Mihajlov4  V. Vujčić1  V. A. Srećković4  M. Malović2 
[1] Faculty of Organizational Sciences, Univesity of Belgrade and Astronomical Observatory, Volgina 7, 11060 Belgrade 74, Serbia.$$;Innovation Centre of Faculty of Technology and Metallurgy, University of Belgrade, Karnegijeva 4, 11000 Belgrade, Serbia.$$;Astronomical Observatory, Volgina 7, 11060 Belgrade 74, Serbia.$$;Institute of Physics, Univesity of Belgrade, P.O. Box 57, 11001, Belgrade, Serbia.$$;Astronomical Observatory, Volgina 7, 11060 Belgrade 74, Serbia and Observatoire de Paris, 92195 Meudon Cedex, France.$$
关键词: Atomic andmolecular processes: photodissociation/association;    chemi-ionization/recombination;    astronomical databases: miscellaneous;    plasmas;    spectral line profiles.;   
DOI  :  
学科分类:天文学(综合)
来源: Indian Academy of Sciences
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【 摘 要 】

MOL-D database is a collection of cross-sections and rate coefficients for specific collisional processes and a web service within the Serbian Virtual Observatory (SerVO) and the Virtual Atomic and Molecular Data Center (VAMDC). This database contains photo-dissociation cross-sections for the individual ro-vibrational states of the diatomic molecular ions and rate coefficients for the atom-Rydberg atom chemiionization and inverse electron–ion–atom chemi-recombination processes. At the moment it contains data for photodissociation crosssections of hydrogen H+2 and helium H+2 molecular ions and the corresponding averaged thermal photodissociation cross-sections. The ro-vibrational energy states and the corresponding dipole matrix elements are provided as well. Hydrogen and helium molecular ion data are important for calculation of solar and stellar atmosphere models and for radiative transport, as well as for kinetics of other astrophysical and laboratory plasma (i.e. early Universe).

【 授权许可】

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