Molecular Astrophysics Laboratory: Star-Forming Regions in the Outer Galaxy (Q84347)

From EU Knowledge Graph
Revision as of 12:36, 14 October 2020 by DG Regio (talk | contribs) (‎Changed label, description and/or aliases in 1 language: translated_label)
Jump to navigation Jump to search
Project in Poland financed by DG Regio
Language Label Description Also known as
English
Molecular Astrophysics Laboratory: Star-Forming Regions in the Outer Galaxy
Project in Poland financed by DG Regio

    Statements

    0 references
    2,193,718.75 zloty
    0 references
    526,492.5 Euro
    13 January 2020
    0 references
    2,193,718.75 zloty
    0 references
    526,492.5 Euro
    13 January 2020
    0 references
    100.0 percent
    0 references
    1 February 2019
    0 references
    31 January 2022
    0 references
    UNIWERSYTET MIKOŁAJA KOPERNIKA
    0 references
    Molecular astrophysics is the interdisciplinary science using molecules in space to characterize physics and chemistry of astronomical objects. In star-forming regions, where stars like our Sun are born in dense, cold cocoons of dust and gas, molecules are often the only means to study the physical processes at play. Their presence and abundances are key to understand chemical evolution of star- and planet-forming material. This knowledge is crucial for understanding how our Solar System, and, ultimately, life on Earth emerged. In this project, we will create the first group in Poland in this new and interdisciplinary discipline that receives enormous attention in the astronomical community and society. We will use the state-of-the-art telescopes to determine the role of environment for star formation. The project is interesting for two companies that will use PI expertise in the infrared detectors and atmospheric models in the development of world-wide networks of telescopes. (Polish)
    0 references
    Molecular Astrophysics is the interdisciplinary science using molecules in space to characterise physics and chemistry of astronomical objects. In star-forming regions, where stars like our Sun are born in dense, cold cocoons of dust and gas, molecules are often the only means to study the physical processes at play. Their presence and abundances are key to understand chemical evolution of star- and planet-forming material. This knowledge is crucial for understanding how our Solar System, and, ultimately, life on Earth emerged. In this project, we will create the first group in Poland in this new and interdisciplinary discipline that receives enormous attention in the astronomical community and society. We will use the state-of-the-art telescopes to determine the role of environment for star formation. The project is interesting for two companies that will use PI expertise in the infrared detectors and atmospheric models in the development of world-wide networks of telescopes. (English)
    14 October 2020
    0 references

    Identifiers

    POIR.04.04.00-00-5D21/18
    0 references