Zobrazeno 1 - 10
of 28
pro vyhledávání: '"Fierlinger Katharina"'
Autor:
Wurm David, Beck Douglas H., Chupp Tim, Degenkolb Skyler, Fierlinger Katharina, Fierlinger Peter, Filter Hanno, Ivanov Sergey, Klau Christopher, Kreuz Michael, Lelièvre-Berna Eddy, Lins Tobias, Meichelböck Joachim, Neulinger Thomas, Paddock Robert, Röhrer Florian, Rosner Martin, Serebrov Anatolii P., Singh Jaideep Taggart, Stoepler Rainer, Stuiber Stefan, Sturm Michael, Taubenheim Bernd, Tonon Xavier, Tucker Mark, Grinten Maurits van der, Zimmer Oliver
Publikováno v:
EPJ Web of Conferences, Vol 219, p 02006 (2019)
The neutron's permanent electric dipole moment dn is constrained to below 3 × 10−26e cm (90% C.L.) [1, 2], by experiments using ultracold neutrons (UCN). We plan to improve this limit by an order of magnitude or more with PanEDM, the first experim
Externí odkaz:
https://doaj.org/article/3f4d675b3af94fc89c2c6f75cc911572
Autor:
Krause, Martin G. H., Burkert, Andreas, Diehl, Roland, Fierlinger, Katharina, Gaczkowski, Benjamin, Kroell, Daniel, Ngoumou, Judith, Roccatagliata, Veronica, Siegert, Thomas, Preibisch, Thomas
Publikováno v:
A&A 619, A120 (2018)
We exploited observational constraints on stars, gas and nucleosynthesis ashes for the closest region of recent massive-star formation, Scorpius-Centaurus OB2, and combined them with 3D hydrodynamical simulations, in order to address physics and hist
Externí odkaz:
http://arxiv.org/abs/1808.04788
Publikováno v:
A&A 599, A94 (2017)
Large-scale shocks formed by clustered feedback of young OB stars are considered an important source of mechanical energy for the ISM and a trigger of molecular cloud formation. Their interaction sites are locations where kinetic energy and magnetic
Externí odkaz:
http://arxiv.org/abs/1701.03696
Autor:
Fierlinger, Katharina M., Burkert, Andreas, Ntormousi, Evangelia, Fierlinger, Peter, Schartmann, Marc, Ballone, Alessandro, Krause, Martin G. H., Diehl, Roland
Stellar winds and supernova (SN) explosions of massive stars ("stellar feedback") create bubbles in the interstellar medium (ISM) and insert newly produced heavy elements and kinetic energy into their surroundings, possibly driving turbulence. Most o
Externí odkaz:
http://arxiv.org/abs/1511.05151
Autor:
Gaczkowski, Benjamin, Preibisch, Thomas, Stanke, Thomas, Krause, Martin G. H., Burkert, Andreas, Diehl, Roland, Fierlinger, Katharina, Kroell, Daniel, Ngoumou, Judith, Roccatagliata, Veronica
Publikováno v:
A&A 584, A36 (2015)
The Lupus I cloud is found between the Upper-Scorpius (USco) and the Upper-Centaurus-Lupus (UCL) sub-groups of the Sco-Cen OB-association, where the expanding USco H I shell appears to interact with a bubble currently driven by the winds of the remai
Externí odkaz:
http://arxiv.org/abs/1509.07368
Autor:
Kretschmer, Karsten, Diehl, Roland, Krause, Martin, Burkert, Andreas, Fierlinger, Katharina, Gerhard, Ortwin, Greiner, Jochen, Wang, Wei
Publikováno v:
A&A 559, A99 (2013)
Massive stars form in groups and their winds and supernova explosions create superbubbles up to kpc in size. Their ejecta are important for the dynamics of the interstellar medium and chemical evolution models. However, ejecta kinematics and the char
Externí odkaz:
http://arxiv.org/abs/1309.4980
Autor:
Krause, Martin, Fierlinger, Katharina, Diehl, Roland, Burkert, Andreas, Voss, Rasmus, Ziegler, Udo
We study the evolution of isolated and merging interstellar bubbles of three stars (25, 32 and 60 M\odot) in a homogeneous background medium with a density of 10 mp /ccm via 3D-hydrodynamic simulations with standard ISM thermodynamics (optically thin
Externí odkaz:
http://arxiv.org/abs/1207.7231
The expansion and collision of two wind-blown superbubbles is investigated numerically. Our models go beyond previous simulations of molecular cloud formation from converging gas flows by exploring this process with realistic flow parameters, sizes a
Externí odkaz:
http://arxiv.org/abs/1011.5751
Autor:
Fierlinger, Katharina M.
Diese Arbeit befasst sich mit dem Einfluss von Sternen, deren Masse acht Sonnenmassen übersteigt, auf das Interstellare Medium in ihrer Umgebung. Solche massereiche Sterne beenden ihr Dasein mit einer Supernovaexplosion und verlieren im Laufe ihrer
Externí odkaz:
http://edoc.ub.uni-muenchen.de/17628/1/Fierlinger_Katharina_M.pdf
http://nbn-resolving.de/urn:nbn:de:bvb:19-176288
http://nbn-resolving.de/urn:nbn:de:bvb:19-176288
Autor:
Jenke, T., Degenkolb, S., Jentschel, M., Nesvizhevsky, V.V., Rebreyend, D., Roccia, S., Soldner, T., Stutz, A., Zimmer, O., Wurm, David, Beck, Douglas H., Chupp, Tim, Degenkolb, Skyler, Fierlinger, Katharina, Fierlinger, Peter, Filter, Hanno, Ivanov, Sergey, Klau, Christopher, Kreuz, Michael, Lelièvre-Berna, Eddy
Publikováno v:
EPJ Web of Conferences; 10/20/2019, Vol. 219, p1-7, 7p