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    Chapter and Conference Paper

    SSSs as progenitors of the BHCs

    In contrast to white dwarfs, neutron stars with near companions can get surrounded by massive accretion disks when their donor stars transfer matter at a greater-than-Eddington rate for sufficiently long. When...

    W. Kundt in Supersoft X-Ray Sources (1996)

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    Chapter and Conference Paper

    Magnetic Field and Differential Rotation of the Sun

    The solar magnetized surface reveals a stable spin period - the Carrington period and a stable oscillation period - the Hale period. The latter is traced by each of the low-order multipole moments, whereby the...

    W. Kundt in The Cosmic Dynamo (1993)

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    Chapter and Conference Paper

    SS 433 — The Preferred Model

    The model for SS 433 which I prefer since the summer of 1979 to all the other proposed models has just been updated (Kundt, 1991). I can therefore be brief. It differs from the standard model in distance (d = 3 k...

    W. Kundt in Stellar Jets and Bipolar Outflows (1993)

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    Chapter and Conference Paper

    The Bipolar-Flow Phenomenon

    Very young stars, known as ‘pre-T-Tauri stars’ or ‘young stellar objects’, tend to be surrounded by elongated outflow regions involving ‘Herbig-Haro objects’. Such ‘bipolar flows’ are reminiscent of the jet-dr...

    W. Kundt in Stellar Jets and Bipolar Outflows (1993)

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    Article

    Buchbesprechungen

    W. Kundt, D. Knorr, K. Bethge in Naturwissenschaften (1991)

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    Article

    Magnetic tensions can control the dynamics of accretion disks

    Magnetic tensions are likely to be the dominant shear force in accretion disks, larger when integrated than turbulent viscosity by an order of magnitude or more. In galactic disks, they guarantee the mass-accr...

    W. Kundt in Astrophysics and Space Science (1990)

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    Article

    Re-analysis of close binary systems

    Line-forming regions around close binaries with strong winds ( \(\dot M\) /4πr * v ≳10−4 g cm−2) are large in extent...

    K. Indulekha, W. Kundt, B. S. Shylaja in Astrophysics and Space Science (1990)

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    Chapter

    Observed Neutron-Star Properties

    The Galaxy contains at least 109 ± 1 neutron stars which are thought to be born in supernova explosions of massive stars, and which we observe as radio pulsars if isolated and as X-ray binaries if attached to a c...

    W. Kundt in Neutron Stars and Their Birth Events (1990)

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    Chapter and Conference Paper

    Supernova structure and light curves

    It is concluded from simple assumptions that:

    1. The SN piston has a relativistic sound speed; a likely realisation of the piston is a mag...

    W. Kundt in Supernova Shells and Their Birth Events (1988)

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    Chapter and Conference Paper

    Interpretation of Supernova Shells

    Our knowledge about Supernova Shells (SNSs) is steadily increasing concerning their number, morphologies and spectra. But there is no general agreement on how to model them. Here I want to comment on their vel...

    W. Kundt in Supernova Shells and Their Birth Events (1988)

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    Chapter and Conference Paper

    Epilogue

    W. Kundt in Supernova Shells and Their Birth Events (1988)

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    Article

    Buchbesprechungen

    P. v. Sengbusch, H. Remmert, H. Scheer, H. Ziegler, L. Jaenicke in Naturwissenschaften (1987)

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    Chapter and Conference Paper

    Magnetic Fields in Supernovae and Supernova Shells

    There are indications that supernova explosions are driven by magnetic springs, i.e. that the spin energy of the collapsing core is transferred to the envelope via magnetic stresses which subsequently convert ...

    W. Kundt in Interstellar Magnetic Fields (1987)

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    Chapter

    The Central Engine

    The literature of the past 10 years has favoured black holes over non-collapsed (super-)massive objects as the central engines of AGN behaviour. But bipolar flows and jets from compact stars are similar and dr...

    W. Kundt in Astrophysical Jets and Their Engines (1987)

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    Chapter

    The Sources and Their Models

    The similarities are stressed between the different astrophysical jet sources, or Bipolar Flows, which apparently make up four classes: Active Galactic Nuclei (=AGN), Young Stellar Objects (=YSO), Binary Neutr...

    W. Kundt in Astrophysical Jets and Their Engines (1987)

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    Chapter

    The Jets

    Jets may simply be the outlets of overpressure bubbles filled with relativistic pair plasma. They ram channels through media of various densities but can be destroyed by neutral intruders, such as photons and ...

    W. Kundt in Astrophysical Jets and Their Engines (1987)

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    Article

    Book review

    Cornelius Hoenselaers, W. Kundt in General Relativity and Gravitation (1986)

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    Article

    Astrophysics and underground physics

    High-energy astrophysics is critically discussed, covering supernova explosions, single and binary neutron stars and active galactic nuclei as well as some acceleration mechanisms like homopolar induction (in ...

    W. Kundt in Il Nuovo Cimento C (1986)

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    Chapter

    Cosmic Ray Acceleration by Binary Neutron Stars

    Young binary neutron stars — the elder brothers of pulsars — are proposed as the boosters of the ionic component of cosmic rays. Their rotational energy can be converted into beams of cosmic rays if there is e...

    W. Kundt in Cosmic Radiation in Contemporary Astrophysics (1986)

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    Article

    Astrophysical boosters

    Constraints are derived on the acceleration of charges in shocks to highly relativistic energies. When applied to the extended extragalactic radio sources and to the cosmic rays, they cast doubt on the mechani...

    W. Kundt in Journal of Astrophysics and Astronomy (1984)

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