96 citations · 594 across the 11 of their papers we have counts for
11 papers
The PanEDM Neutron Electric Dipole Moment Experiment at the ILL
David Wurm, Douglas H. Beck, Tim Chupp +24
The neutron's permanent electric dipole moment is constrained to below (90% C.L.) [ arXiv:hep-ex/0602020, arXiv:1509.04411 ], by experiments usi…
Surround & Squash: The Interstellar Medium around Scorpius Centaurus OB2
Martin G. H. Krause, Andreas Burkert, Roland Diehl +7
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 wi…
Squeezed between shells? On the origin of the Lupus I molecular cloud. - II. APEX CO and GASS HI observations
B. Gaczkowski, V. Roccatagliata, S. Flaischlen +7
[Abridged] The Lupus I cloud is found between the Upper-Scorpius and the Upper-Centaurus-Lupus sub-groups, where the expanding USco HI shell appears to interact with a bubble curre…
The role of magnetic fields in the structure and interaction of supershells
Evangelia Ntormousi, Joanne R. Dawson, Patrick Hennebelle +1
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. Th…
Stellar feedback efficiencies: supernovae versus stellar winds
Katharina M. Fierlinger, Andreas Burkert, Evangelia Ntormousi +5
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 kinet…
Squeezed between shells? On the origin of the Lupus I molecular cloud. APEX/LABOCA, Herschel, and Planck observations
Benjamin Gaczkowski, Thomas Preibisch, Thomas Stanke +7
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 appear…
A large-scale magnetic shield with 10^6 damping at mHz frequencies
I. Altarev, M. Bales, D. H. Beck +16
We present a magnetically shielded environment with a damping factor larger than one million at the mHz frequency regime and an extremely low field and gradient over an extended vo…
A Young GMC Formed at the Interface of Two Colliding Supershells: Observations Meet Simulations
J. R. Dawson, E. Ntormousi, Y. Fukui +2
Dense, star-forming gas is believed to form at the stagnation points of large-scale ISM flows, but observational examples of this process in action are rare. We here present a gian…
Kinematics of massive star ejecta in the Milky Way as traced by 26Al
Karsten Kretschmer, Roland Diehl, Martin Krause +5
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…
Feedback by massive stars and the emergence of superbubbles I. Energy efficiency & Vishniac instabilities
Martin Krause, Katharina Fierlinger, Roland Diehl +3
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-hyd…
Formation of Cold Filamentary Structure from Wind Blown Superbubbles
Evangelia Ntormousi, Andreas Burkert, Katharina Fierlinger +1
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 f…