Results 81 to 90 of about 372 (130)
While plane-of-sky magnetic field observations in molecular clouds are now common, observations of their line-of-sight magnetic field remain limited. To address this issue, M. Tahani et al. developed a technique based on Faraday rotation.
Mehrnoosh Tahani +5 more
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Interstellar Magnetic Fields: An Observational Perspective
Abstract: Chapter 1 establishes the plausibility of “magnetic molecular clouds.” We show that the empirically known relations between spectral line width, density, and cloud size can be derived from a virial equilibrium model where gravity is balanced by the sum of magnetic and pressure support.
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Observing the interstellar magnetic field
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.
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Despite the pervasive nature of interstellar dust and its impact on nearly all observations, most dust corrections employ line-of-sight averages over large angular scales.
Jordan A. Bartlett, Henry A. Kobulnicky
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Study of Magnetic Field and Turbulence in the TeV Halo around the Monogem Pulsar
Magnetic fields are ubiquitous in the interstellar medium, including extended objects such as supernova remnants and diffuse halos around pulsars. Its turbulent characteristics govern the diffusion of cosmic rays and the multiwavelength emission from ...
Sunil Malik, Ka Ho Yuen, Huirong Yan
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On Interstellar Grain Alignment by a Magnetic Field [PDF]
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Interstellar Polarization and Magnetic Fields.
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Planetary nebulae and the interstellar magnetic field [PDF]
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The Local Irregularities of the Interstellar Magnetic Field [PDF]
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Interstellar Lines and the Dissipation of Interstellar Magnetic Fields by Petschek's Mechanism.
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