Herschel spectral-line mapping of the HH211 protostellar system

Mid- and far-infrared observations of the environment around embedded protostars reveal a plethora of high excitation molecular and atomic emission lines. In this paper recently accepted for publication in Astronomy & Astrophysics we present spectro-imaging observations of the HH211 system with Herschel/PACS that record emission from major molecular (CO, H2O and OH) and atomic coolants […]

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Public talk at the WAA \”Der Mechanismus von Antikythera\”

I am excited to give an invited talk on the Antikythera mechanism at the Vienna Amateur Astronomers club (Wiener Arbeitsgemeinschaft for Astronomie). The topic of the presentation combines in a unique way astronomy with  history and archeology, which are some of my major fields of interest. Ancient civilization is mainly related to and studied through arts and

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EWASS 2017, Prague: Symposium \” Astrophysical Jets and Outflows – from compact objects to protostars\”

I am proud to co-organize with excellent colleagues for the second consecutive year a symposium on astrophysical jets and outflows within the framework of the European Week of Astronomy and Space Science (EWASS), held this year in Prague, Czech Republic between 26-30 of June 2017. For more information and registration you can directly visit the EWASS

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Feedback of atomic jets from embedded protostars in NGC1333

The star-formation feedback onto the parent cloud is conventionally examined through the study of molecular outflows. Little is however known on the effect that atomic ejecta, tracing fast shocks, can have on the global cloud properties. In this study we employ Herschel/PACS [OI] and [CII] spectral line maps of the NGC 1333 star-forming region to assess the

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FFG funding awarded

Our project JetPro* has been awarded full funding from the Austrian Research Promotion Agency (FFG) in the framework of the 12th Austrian Space Applications Programme (ASAP). In the following years we will have the opportunity to study the influence of protostellar ejecta during the star-formation process on determining the final mass of forming stars but also shape their

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