Eva Wirström
Eva Wirström is a Associate professor and Division Head for the Onsala Space Observatory division. Her research interests includes the physics and chemistry in the giant clouds of gas and dust forming stars and planetary systems in our galaxy, as well as the link between these and the emergence of life - astrochemistry and astrobiology. As senior researcher she works on the Science team for one of the instruments bound for the Jupiter system in ESA's JUICE (JUpiter ICy moons Explorer) mission, the Submillimetre Wave Instrument (SWI). SWI will be used to observe the thin water atmospheres of Jupiter's largest moons, connected to Eva's previous work on interpreting data from the Herschel Space Observatory, which observed the water content in many different kinds of space environments.
Eva's research is funded by the Swedish National Space Board.
Showing 34 publications
Effect of the 3D distribution on water observations made with the SWI: I. Ganymede
Complex Organic Molecules in Star-Forming Regions of the Magellanic Clouds
Revised Models of Interstellar Nitrogen Isotopic Fractionation
Doubly 15N-substituted diazenylium: THz laboratory spectra and fractionation models
Chemical complexity induced by efficient ice evaporation in the Barnard 5 molecular cloud
HCN observations of comets C/2013 R1 (Lovejoy) and C/2014 Q2 (Lovejoy)
A Search for O2 in Co-Depleted Molecular Cloud Cores with Herschel
FORMATION AND RECONDENSATION OF COMPLEX ORGANIC MOLECULES DURING PROTOSTELLAR LUMINOSITY OUTBURSTS
On the Nature of the Enigmatic Object IRAS 19312+1950: A Rare Phase of Massive Star Formation?
Cometary Isotopic Measurements
The Composition of the Protosolar Disk and the Formation Conditions for Comets
15N fractionation in star-forming regions and Solar System objects
COLD WATER VAPOR IN THE BARNARD 5 MOLECULAR CLOUD
Using Methanol Beacons to Find Water in the Dark
Depletion Cores - the O2 hideout?
A Radio Astronomical Star Party for those "On The Verge"
On the ubiquity of molecular anions in the dense interstellar medium
Organic chemistry of low-mass star-forming cores I: 7 mm spectroscopy of Chamaeleon MMS1
Observations of Carbon Isotopic Fractionation in Interstellar Formaldehyde
The 12C/13C ratio as a chemistry indicator
Observational tests of interstellar methanol formation
Ground-state ammonia and water in absorption towards Sgr B2
Observational constraints on the formation of interstellar methanol
A search for pre-biotic molecules in hot cores
Observations of chemical differentiation in clumpy molecular clouds
Odin * CO and 13CO J=5-4 mapping of Orion KL - a step towards accurate water abundances
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Showing 5 research projects
ISSI Team "Provenances of our Solar System’s relics"
Swedish science support for Juice/SWI
Swedish science support for SWI (Submillimetre Wave Instrument)
Interstellar Chemistry with Herschel