about
A dark jet dominates the power output of the stellar black hole Cygnus X-1.A Fundamental Plane of black hole activityHiding in Plain Sight:ChandraObservations of the Quiescent Neutron Star 4U 2129+47 in EclipseThe youngest known X-ray binary: Circinus X-1 and its natal supernova remnantMultiwavelength observations of the SS 433 jetsMODELING THE SS 433 JET BENDSModeling the Relativistic Jets in SS 433 Using Chandra X-ray SpectroscopyMassive compact galaxies with high-velocity outflows: morphological analysis and constraints on AGN activityShock heating by Fanaroff-Riley type I radio sources in galaxy clustersTesting black hole jet scaling relations in low-luminosity active galactic nucleiSUB-mm JET PROPERTIES OF THE X-RAY BINARY SWIFT J1745–26An evolving compact jet in the black hole X-ray binary MAXI J1836-194Disc-jet coupling in the 2009 outburst of the black hole candidate H1743−322Evolution of the Radio-X-ray coupling throughout an entire outburst of Aquila X-1Investigating accretion disk – radio jet coupling across the stellar mass scaleThe complete spectrum of the neutron star X-ray binary 4U 0614+091A radio-emitting outflow in the quiescent state of A0620−00: implications for modelling low-luminosity black hole binariesA multiwavelength study of Cygnus X-1: the first mid-infrared spectroscopic detection of compact jetsIs the “IR Coincidence” Just That?Long term variability of Cygnus X-1Global simulations of the interaction of microquasar jets with a stellar wind in high-mass X-ray binariesJet–Environment Interactions as Diagnostics of Jet PhysicsSimulations of bent-double radio sources in galaxy groupsExploring Regimes in Black Hole ScalingEvolution of Active Galactic NucleiAll curled up: a numerical investigation of shock-bubble interactions and the role of vortices in heating galaxy clustersJet trails and mach cones: the interaction of microquasars with the interstellar mediumLuminosity functions and point-source properties from multiple Chandra observations of M81XIM--a virtual X-ray observatory: investigating the X-ray appearance and line profile function of vortex rings in galaxy clustersSwimming against the current: simulations of central AGN evolution in dynamic galaxy clustersParsec-scale bipolar X-ray shocks produced by powerful jets from the neutron star Circinus X-13C28 in Abell 115- A Radio Source With a TwistProspects of high-resolution X-ray spectroscopy for active galactic nucleus feedback in galaxy clustersA parsec scale X-ray extended structure from the X-ray binary Circinus X−1Discovery of a large and bright bow shock nebula associated with low-mass X-ray binary SAX J1712.6−3739Evolution of X-ray cavitiesBlazing Trails: Microquasars as Head‐Tail Sources and the Seeding of Magnetized Plasma into the ISMA synthesis model for AGN evolution: supermassive black holes growth and feedback modesA DeepChandraObservation of Abell 4059: A New Face to “Radio‐Mode” AGN Feedback?How Deep is Your Lobe? Microquasars and Their Impact on the ISM
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description
Duits astronoom
@nl
astronome allemand
@fr
astronomo alemaniarra
@eu
astronomo tedesco
@it
astrònom alemany
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astrónomo alemán
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astrónomo alemán
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astrónomu alemán
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astrônomo alemão
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name
Sebastian Heinz
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Sebastian Heinz
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Sebastian Heinz
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Sebastian Heinz
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Sebastian Heinz
@sl
Sebastian Heinz
@sq
type
label
Sebastian Heinz
@ast
Sebastian Heinz
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Sebastian Heinz
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Sebastian Heinz
@nl
Sebastian Heinz
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Sebastian Heinz
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prefLabel
Sebastian Heinz
@ast
Sebastian Heinz
@en
Sebastian Heinz
@es
Sebastian Heinz
@nl
Sebastian Heinz
@sl
Sebastian Heinz
@sq
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P106
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P214
P31
P496
0000-0002-8433-8652
P512
P734
P735
P7859
viaf-80854222