Pooneh Nazari

ESO & IAU Gruber Fellow

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Observations

My observational studies focus on using ALMA and JWST to observe the molecules in the gas and ice around protostars. One of my recent studies focused on observations of complex cyanides in ices with JWST-NIRSpec. We tentatively detected methyl cyanide, ethyl cyanide, and nitrous oxide for the first time in interstellar ices around three protostars (see publications).


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Modelling

I have worked on several modelling projects (see publications). Here I show a graph comparing the integrated line fluxes of methanol calculated by RADMC-3D with observations of low-mass protostars in Perseus. In this work I studied an envelope-only and an envelope-plus-disk model. We concluded that disks and optically thick dust are necessary to explain the lack of methanol emission at millimetre wavelengths in some protostars. For more information feel free to check out the paper.


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Address


Office E.3.46, ESO Headquarters, Karl-Schwarzschild-Strasse 2, 85748, Garching