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Mol-D a Database and a Web Service within the Serbian Virtual Observatory and the Virtual Atomic and Molecular Data Centre

Published online by Cambridge University Press:  30 May 2017

Vladimir A. Srećković Open the ORCID record for Vladimir A. Srećković [Opens in a new window] ,
Darko Jevremović ,
Veljko Vujčić ,
Ljubinko M. Ignjatović ,
Nenad Milovanović ,
Sanja Erkapić  and
Milan S. Dimitrijević
Vladimir A. Srećković
Affiliation:
Institute of Physics Belgrade, University of Belgrade, P.O. Box 57, 11001, Belgrade, Serbia email: vlada@ipb.ac.rs
Darko Jevremović
Affiliation:
Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia email: darko@aob.rs
Veljko Vujčić
Affiliation:
Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia email: darko@aob.rs Faculty of Organizational Sciences, Univesity of Belgrade, Serbia
Ljubinko M. Ignjatović
Affiliation:
Institute of Physics Belgrade, University of Belgrade, P.O. Box 57, 11001, Belgrade, Serbia email: vlada@ipb.ac.rs
Nenad Milovanović
Affiliation:
Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia email: darko@aob.rs
Sanja Erkapić
Affiliation:
Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia email: darko@aob.rs
Milan S. Dimitrijević
Affiliation:
Astronomical Observatory, Volgina 7, 11060 Belgrade, Serbia email: darko@aob.rs Observatoire de Paris, 92195 Meudon Cedex, France email: mdimitrijevic@aob.rs IHIS Techno experts, Batajnički put 23, 11080 Zemun, Serbia
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Abstract

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In this contribution we report the current stage of the MOLecular Dissociation (MOL-D) database which is a web service within the Serbian virtual observatory (SerVO) and node within Virtual Atomic and Molecular Data Center (VAMDC). MOL-D is an atomic and molecular (A&M) database devoted to the modelling of stellar atmospheres, laboratory plasmas, industrial plasmas etc. The initial stage of development was done at the end of 2014, when the service for data connected with hydrogen and helium molecular ions was done. In the next stage of the development of MOL-D, we include new cross-sections and rate coefficients for processes which involve species such as XH+, where X is atom of some metal. Data are important for the exploring of the interstellar medium as well as for the early Universe chemistry and for the modeling of stellar and solar atmospheres. In this poster, we present our ongoing work and plans for the future.

Keywords

Virtual ObservatoryAstroinformaticsStarsAtomic and Molecular DataDatabases
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 12 , Symposium S325: Astroinformatics , October 2016 , pp. 393 - 396
Copyright
Copyright © International Astronomical Union 2017 

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