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

Abstract

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.

References in corpus (8)

• The Sloan Digital Sky Survey: Technical Summary
• Ion-atom radiative processes in the solar atmosphere: quiet Sun and sunspots
• The ion-atom absorption processes as one of the factors of the influence on the sunspot opacity
• The non-symmetric ion-atom radiative processes in the stellar atmospheres
• Absorption non-symmetric ion-atom processes in helium-rich white dwarf atmospheres
• MOL-D: A Collisional Database and Web Service within the Virtual Atomic and Molecular Data Center
• State-to-state vibrational kinetics of H${}_2$ and H${}_2^{+}$ in a post-shock cooling gas with primordial composition
• Astroinformatics, data mining and the future of astronomical research