Results 1 to 10 of about 37,251 (259)
Interstellar Magnetic Field [PDF]
Nature, 1968 Roger and Shuter1 have pointed out that the recent measurement (Smith2) of the interstellar magnetic field from the Faraday rotation of the plane polarized radio waves from the pulsar CP 0950 may be interpreted as a combination of ionospheric and interstellar rotation.
R. S. ROGER, W. L. H. SHUTER
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Heliosphere in a strong interstellar magnetic field [PDF]
Journal of Physics: Conference Series, 2017 We present results of MHD simulations of the global structure of the heliosphere for a wide range of the interstellar magnetic field (ISMF) strengths (2-20 µG). For a strong interstellar field, the plasma flow in and around the heliosphere as well as the magnetic field draped over the heliopause have a simple structure, reminiscent of (though not ...
A Czechowski, J Grygorczuk
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Shape and evolution of wind-blown bubbles of massive stars: on the effect of the interstellar magnetic field [PDF]
, 2015 The winds of massive stars create large (>10 pc) bubbles around their progenitors. As these bubbles expand they encounter the interstellar coherent magnetic field which, depending on its strength, can influence the shape of the bubble.
Marcowith, Alexandre +2 more
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Dynamically dominant magnetic fields in the diffuse interstellar medium [PDF]
, 2009 Observations show that magnetic fields in the interstellar medium (ISM) often do not respond to increases in gas density as would be naively expected for a frozen-in field. This may suggest that the magnetic field in the diffuse gas becomes detached from
A. Shukurov +5 more
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Magnetic Fields in the Interstellar Medium
, 2017 The interstellar medium – the space between the stars in our Galaxy – is multiphase, turbulent, and magnetic. Magnetism in the interstellar medium is difficult to observe and to simulate, and the study of interstellar magnetic fields is riddled with open questions. In this Thesis we make progress in several important areas.
Susan E. Clark
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Observing the interstellar magnetic field
, 1968 Before coming to a more detailed discussion, let us see what ways exist to establish the presence of a magnetic field In the galaxy at all. (Table 1). We shall briefly review these methods one by one.
H. C. van de Hulst
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Magnetic fields and UHECR propagation [PDF]
EPJ Web of Conferences, 2023 I review the main observational tools used to detect and measure magnetic fields in the interstellar medium of our Galaxy (considering both the Galactic disk and the Galactic halo), in the interstellar medium of external galaxies, and in the ...
Ferrière Katia
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A Large Magnetic Hump in the VLISM Observed by Voyager 1 in 2020–2022
The Astrophysical Journal, 2023 Voyager 1 has been moving through the very local interstellar medium (VLISM) for approximately one solar cycle, from 122.58 au on 2012/DOY 238 (August 25) to 158.5 au on 2023.0. Previously, an abrupt increase (“jump”) in the magnetic field strength B and
L. F. Burlaga +5 more
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SOFIA Observations of 30 Doradus. II. Magnetic Fields and Large-scale Gas Kinematics
The Astrophysical Journal, 2023 The heart of the Large Magellanic Cloud, 30 Doradus, is a complex region with a clear core-halo structure. Feedback from the stellar cluster R136 has been shown to be the main source of energy creating multiple parsec-scale expanding-shells in the outer ...
Le Ngoc Tram +15 more
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Magnetic Misalignment of Interstellar Dust Filaments
The Astrophysical Journal, 2023 We present evidence for scale-independent misalignment of interstellar dust filaments and magnetic fields. We estimate the misalignment by comparing millimeter-wave dust-polarization measurements from Planck with filamentary structures identified in ...
Ari J. Cukierman +2 more
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