Results 91 to 100 of about 35,066 (146)

The investigation of the hierarchical structure of the interstellar magnetic fields [PDF]

, 1991
A.L. Lazarian
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Magnetically Aligned Striations in the L914 Filamentary Cloud

The Astronomical Journal
We present CO( J = 1–0) multiline observations toward the L914 dark cloud in the vicinity of the Cygnus X region, using the 13.7 m millimeter telescope of the Purple Mountain Observatory.
Li Sun, Xuepeng Chen, Min Fang, Shaobo Zhang, Yan Gong, Jiancheng Feng, Xuefu Li, Qing-Zeng Yan, Ji Yang   +8 more
doaj   +1 more source

A reexamination of “interstellar ion waves” previously identified in Pioneer 10 magnetic field data [PDF]

, 1998
Neil Murphy, E. J. Smith, Joyce Wolf, D. S. Intriligator   +3 more
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What Rogue Hydrogen Clouds Tell Us about Galactic Magnetic Fields

The Astrophysical Journal
Observations of the Milky Way and external galaxies support the idea that large-scale magnetic fields are concentrated in galactic disks, with halo magnetic fields at least an order of magnitude weaker.
Bailey M. Forster, Tyler J. Foster, Roland Kothes, Alex S. Hill, Jo-Anne C. Brown   +4 more
doaj   +1 more source

Magnetic Fields and the Interstellar Medium in Spiral Arms [PDF]

, 1996
M. Urbaník, M. Soida, R. Beck
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A Search for Variable Interstellar Magnetic Fields and Neutron Star Precession in Four Years of Polarization Position Angle Measurements on 98 Pulsars [PDF]

, 2000
J. M. Weisberg, J. J. Morgan, J. T. Despotes, J. E. Everett, J. M. Cordes   +4 more
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Interstellar Hydroxyl Masers in the Galaxy. II. Zeeman Pairs and the Galactic Magnetic Field [PDF]

, 2003
Vincent L. Fish, M. J. Reid, A. L. Argon, K. M. Menten   +3 more
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Equilibrium configurations of the interstellar medium layers in the presence of magnetic field and gravitation [PDF]

, 2003
В. А. Антонов, O. A. Zheleznyak
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Faraday Tomography with CHIME: The “Tadpole” Feature G137+7

The Astrophysical Journal
A direct consequence of Faraday rotation is that the polarized radio sky does not resemble the total intensity sky at long wavelengths. We analyze G137+7, which is undetectable in total intensity but appears as a depolarization feature.
Nasser Mohammed, Anna Ordog, Rebecca A. Booth, Andrea Bracco, Jo-Anne C. Brown, Ettore Carretti, John M. Dickey, Simon Foreman, Mark Halpern, Marijke Haverkorn, Alex S. Hill, Gary Hinshaw, Joseph W. Kania, Roland Kothes, T. L. Landecker, Joshua MacEachern, Kiyoshi W. Masui, Aimee Menard, Ryan R. Ransom, Wolfgang Reich, Patricia Reich, J. Richard Shaw, Seth R. Siegel, Mehrnoosh Tahani, Alec J. M. Thomson, Tristan Pinsonneault-Marotte, Haochen Wang, Jennifer L. West, Maik Wolleben, Dallas Wulf, CHIME and GMIMS Collaborations   +30 more
doaj   +1 more source

Three‐dimensional Features of the Outer Heliosphere Due to Coupling between the Interstellar and Interplanetary Magnetic Fields. I. Magnetohydrodynamic Model: Interstellar Perspective [PDF]

, 2004
N. V. Pogorelov, G. P. Zank, Tatsuki Ogino   +2 more
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