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- W2898403780 abstract "Organic molecules are the building blocks of life and this is why the search for amino acids and their complex organic precursors at different stages of star and planet formation is one of the exciting topics in modern astronomy. Understanding how, when and where organics (simple as well as complex including potentially prebiotic molecules) are formed is one of the most important questions for Astrochemistry/Astrobiology. Complex organics have been detected in prestellar cores, protostars, and protoplanetary disks. Can a part of the organic content observed in these regions be preserved during the protostellar stages and incorporated into asteroids and comets, that can deliver it to planetary embryos through impacts? By looking at the cometary compositions, observations of solar-type protostars can help to address this critical question. In this context, here we will present our observations towards the solar-type protostar IRAS 16293-2422 in the 3mm band of the IRAM 30m telescope along with existing ALMA observations. We will also describe how the chemo-dynamical simulations using the state-of-the-art gas-grain-bulk chemical-kinetic model can help us to understand the chemical composition of comet 67P observed by Rosetta. For the first time, we will also shed light on to the possibility of protostellar inheritance of glycine (king of the ROSETTA Zoo) on to the comet 67P." @default.
- W2898403780 created "2018-11-02" @default.
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- W2898403780 date "2018-07-14" @default.
- W2898403780 modified "2023-09-27" @default.
- W2898403780 title "The chemical link between comet 67P/C-G and low mass protostar IRAS 16293-2422: Integrative Studies in Observational Astronomy and Chemical-Dynamical Modeling" @default.
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