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[PDF] Top 20 Modelling neutron star magnetic fields

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Modelling neutron star magnetic fields

Modelling neutron star magnetic fields

... the magnetic field contains a strong azimuthal ...the star, while the gradient of the electron number density is parallel to the ...latitudes. Magnetic fields containing more energy in the ... See full document

6

Modelling the spin pulse profile of the isolated neutron star RX J0720.4-3125 observed with XMM-Newton

Modelling the spin pulse profile of the isolated neutron star RX J0720.4-3125 observed with XMM-Newton

... isolated neutron star ...the neutron star is heated by accretion, and place limits on the mag- netic field ...stars: neutron, stars: magnetic fields, individual: ... See full document

6

Search for Gravitational Waves from a Nearby Neutron Star Using Barycentric Resampling

Search for Gravitational Waves from a Nearby Neutron Star Using Barycentric Resampling

... be neutron star-neutron star or neutron star-black hole ...be neutron stars with huge magnetic fields which flare up from time to time and emit prodigious ... See full document

174

Magnetic Axis Drift and Magnetic Spot Formation in Neutron Stars with Toroidal Fields

Magnetic Axis Drift and Magnetic Spot Formation in Neutron Stars with Toroidal Fields

... of magnetic spots. In principle the magnetic field evolution is coupled to its thermal evolution, as conductivity is a func- tion of temperature (Chugunov ...the magnetic field and consequently ... See full document

13

Spin period change and the magnetic fields of neutron stars in Be X-ray binaries in the SMC

Spin period change and the magnetic fields of neutron stars in Be X-ray binaries in the SMC

... From the parameters of each system, we determine whether each neutron star is accreting via a disc or wind. An accretion disc will form if the net angular momentum per unit mass of accreted matter J, is too ... See full document

6

The X-ray pulsar 2A 1822-371 as a super-Eddington source

The X-ray pulsar 2A 1822-371 as a super-Eddington source

... The neutron star primary accretes material from a ...main-sequence star (Harlaftis, Charles & Horne 1997), and the system has a binary orbit of ...through modelling of the light curve ... See full document

11

General relativistic magnetohydrodynamic simulations of binary neutron star mergers

General relativistic magnetohydrodynamic simulations of binary neutron star mergers

... binary neutron star (BNS) mergers, conducted by using the numerical code ...for neutron matter is APR4 and both magnetized and unmagnetized cases are ...different magnetic field orientations ... See full document

90

The Magnetospheres of (Accreting) Neutron Stars - Observational Clues

The Magnetospheres of (Accreting) Neutron Stars - Observational Clues

... measure neutron star magnetic fields, but in addition observations of cyclotron lines also allow us to test the models for the accretion flow onto neutron stars discussed ... See full document

10

An Accretion Model for Anomalous X‐Ray Pulsars

An Accretion Model for Anomalous X‐Ray Pulsars

... are neutron stars with magnetic fields similar to those of radio pulsars, accreting from binary companions of very low ...old neutron star accreting from the interstellar ... See full document

18

Magnetic field evolution in magnetar crusts through three dimensional simulations

Magnetic field evolution in magnetar crusts through three dimensional simulations

... strong magnetic fields to explain their ob- served quiescent and bursting emission, implying that the field strength within the star’s outer crust is orders of magnitude larger than the dipole component ... See full document

8

An Algorithm for the Simulation of the Magnetized Neutron Star Cooling

An Algorithm for the Simulation of the Magnetized Neutron Star Cooling

... magnetized neutron stars cooling process is an interesting subject for the investi- gations of the internal structure of such ...The magnetic field of compact object when it is more than 10 14 G has a ... See full document

6

Exotic atoms at extremely high magnetic fields: the case of neutron star atmosphere

Exotic atoms at extremely high magnetic fields: the case of neutron star atmosphere

... the star, and it spans more than 10 orders of magnitudes in the range of a dozen ...the star and the radial fraction of di ff erent baryonic and leptonic species in a NS for a given EoS is shown in ...a ... See full document

10

Neutron stars velocities and magnetic fields

Neutron stars velocities and magnetic fields

... explain neutron stars velocities due to the anisotropic emission of ...Strong magnetic fields present in neutron stars are the source of the anisotropy in the ...the neutron star ... See full document

7

Disk accretion onto a magnetized star

Disk accretion onto a magnetized star

... a magnetic field. Moving across the magnetic field, the plasma gets polarized and creates the large scale electric field ...E fields at the same velocity v not slowing ...a star surface, on ... See full document

6

The Balloon-Borne Large Aperture Submillimeter Telescope for Polarimetry (Blast-Pol)

The Balloon-Borne Large Aperture Submillimeter Telescope for Polarimetry (Blast-Pol)

... MHD star formation theories suggest that a self-gravitating cloud can be supported by a purely static field [Stahler and Palla, 2005]; flux freezing within molecular clouds signifies that the magnetic field ... See full document

216

Walch, Stefanie
  

(2008):


	The formation and early evolution of protostellar disks around low-mass stars..


Dissertation, LMU München: Fakultät für Physik

Walch, Stefanie (2008): The formation and early evolution of protostellar disks around low-mass stars.. Dissertation, LMU München: Fakultät für Physik

... the star formation process and to link its initial and final ...dust, magnetic fields and tur- bulence, while at the same time overcoming 17 orders of magnitude in density and 10 orders of magnitude ... See full document

185

Enhanced Phenomena in Metals with Electric and Magnetic Fields: II Magnetic Fields

Enhanced Phenomena in Metals with Electric and Magnetic Fields: II Magnetic Fields

... magnetic annealing in a field of 13 T increased the {110}[001] Goss texture even above the Curie temperature. Martikainen and Lindroos 6) noted another important effect of magnetic field, that is, the ... See full document

5

The Dynamics of the Neutron Complexes: From Neutron Star to Black Hole

The Dynamics of the Neutron Complexes: From Neutron Star to Black Hole

... 1. On a small cosmological scale, i.e. at Galactic distances, it is confirmed the Newtonian law of gravity, i.e. the attraction of massive particles of the environment to a given particle (neutron). An effective ... See full document

5

Formation and Evolution of Neutron Star Binaries: Masses of Neutron Stars

Formation and Evolution of Neutron Star Binaries: Masses of Neutron Stars

... independent of the maximum mass of NS, but the result of evolution of NS binaries. We discuss that NS-NS binaries are formed when the initial mass di ff erence of two progenitors of double neutron stars is less ... See full document

6

Probing neutron star physics using accreting neutron stars

Probing neutron star physics using accreting neutron stars

... accreting neutron stars systems as probes of neutron star ...accreting neutron stars during ...these neutron stars do not show evidence of spin variations during the ...accreting ... See full document

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