6篇
您的检索式：作者名="Heber Ulrich"
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| 1 | Protein-sparing therapy in the postoperative period显示文摘 | Ulrich Keller M.D. Didier Clerc M.D. Marius Kr?nzlin M.D. M. Heberer M.D | 1986 | World Journal of Surgery1986，，1： | 2 |
| 2 | Irrungen, Wirrungen? The Mehler reaction in relation to cyclic electron transport in C3 plants显示文摘 | Ulrich Heber | 2002 | Photosynthesis Research (-)2002，，1： | 1 |
| 3 | Inhibition of photosynthesis, acidification and stimulation of zeaxanthin formation in leaves by sulfur dioxide and reversal of these effects显示文摘 | Sonja Veljovic-Jovanovic Wolfgang Bilger Ulrich Heber | 1993 | Planta1993，，3： | 1 |
| 4 | Hot subdwarf stars 显示文摘 | Heber Ulrich | 2009 | A&A2009，47，： | 1 |
| 5 | Flexible coupling between light-dependent electron and vectorial proton transport in illuminated leaves of C3 plants. Role of photosystem I-dependent proton pumping显示文摘 | Gabriel Cornic Nicolai G. Bukhov Christian Wiese Richard Bligny Ulrich Heber | 2000 | Planta2000，，3： | 1 |
| 6 | Three new late-type hypervelocity star candidates from Gaia DR2 with refined selection criteria显示文摘Several dozen hypervelocity star(HVS)candidates have been reported based on the second data release of Gaia(Gaia DR2).However,it has been proven that the radial velocities of some Gaia HVS candidates are not reliable.In this paper,we employ refined astrometric criteria to re-examine Gaia DR2,arriving at a more reliable sample of HVS and high velocity star candidates than those found by previous authors.We develop a method called Binary Escape Probability Analysis to identify some HVS candidates.This method allows us to work with stars having only two epochs of measured radial velocity.These stars were usually discarded in previous similar studies.A scrutiny of our final results sheds light on selection effects present in our studies,which we propose to be the focus of future studies.In total,we find three late-type(2 G-type and 1 K-type)HVS and 21 high velocity star candidates,3 and 11 of which are new,respectively.Judging by their historical trajectories,which we calculate,all three HVS candidates could not have had Galactic center origins.Further monitoring is required to confirm their status. | Jiao Li Shi Jia Yan Gao Deng-Kai Jiang Thomas Kupfer Ulrich Heber Chao Liu Xue-Fei Chen Zhan-Wen Han | 2020 | Research in Astronomy and Astrophysics2020，20，3： | 0 |
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