Why are ulrich and georg feulner

Niv Drory. Ulrich Hopp. Jan Snigula. Gary J. Select Format Select format. Permissions Icon Permissions. Issue Section:. Download all slides. View Metrics. Email alerts Article activity alert. Advance article alerts. New issue alert. He teaches at the University of Potsdam where he obtained his Habilitation in Georg's research focuses on climate modelling, deep-time paleoclimatology in particular the climate on early Earth, Snowball Earth episodes, past greenhouse climates and climate changes during mass-extinction events as well as present and future climate change.

My research in climate science covers a broad range of topics. In terms of methodology, my research is primarily based on numerical models of the coupled Earth system, complemented by data analysis and theoretical arguments. Web of Science citation summary: 3, citations, h index 30, i. Evidence for size evolution? In: A. Banday, S. Bartelmann eds.

Ida Pfeiffer Visiting Professor at the University of Vienna, full-term lectures on climate modelling and Earth's climate history summer term Potsdam Institute for Climate Impact Research. Furthermore, these highest mass galaxies contain the oldest stellar populations at all redshifts. The line of maximum SSFR runs parallel to lines of constant star formation rate. We also show that the large SSFRs of low-mass galaxies cannot be sustained over extended periods of time. Finally, our results do not require a substantial contribution of merging to the growth of stellar mass in massive galaxies over the redshift range probed.

We note that highly obscured galaxies which remain undetected in our sample do not affect these findings for the bulk of the field galaxy population. Oxford University Press is a department of the University of Oxford.

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