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

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