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Several mechanisms have been proposed to explain the alignment of grains with the interstellar magnetic field, including paramagnetic dissipation, radiative torques, and supersonic gas-grain streaming. These must compete with disaligning…

天体物理学 · 物理学 2008-11-26 Joseph C. Weingartner

Interstellar polarization in the optical/infrared has long been known to be due to asymmetrical dust grains aligned with the magnetic field and can potentially provide a resource effective way to probe both the topology and strength of the…

星系天体物理 · 物理学 2012-08-23 B. -G. Andersson

Thermal fluctuations in the magnetization of interstellar grains will produce magnetic dipole emission at frequencies below ~100 GHz. We show how to calculate absorption and emission from small particles composed of magnetic materials. The…

天体物理学 · 物理学 2009-10-30 B. T. Draine , A. Lazarian

Interstellar dust grains exhibit complex dynamics which is essential for understanding many key interstellar processes that involve dust, including grain alignment, grain growth, grain shattering etc. Grain rotational and translational…

天体物理学 · 物理学 2007-05-23 A. Lazarian , Huirong Yan

Grain alignment theory suggests that grains should be aligned in circumstellar regions and the observational data available supports this conclusion. We discuss the alignment of grains via (1) magnetic relaxation, (2) mechanical processes,…

天体物理学 · 物理学 2007-05-23 Lazarian A

Polarimetry is one of the most informative techniques of studying magnetic fields in molecular clouds. How reliable the interpretation of the polarization maps in terms of magnetic fields is the issue that the grain alignment theory…

天体物理学 · 物理学 2016-08-30 A. Lazarian , J. Cho

Radiative torques on irregular dust grains, in addition to producing superthermal rotation, play a direct dynamical role in the alignment of interstellar dust with the local magnetic field. The equations governing the orientation of…

天体物理学 · 物理学 2009-10-28 B. T. Draine , Joseph C. Weingartner

The motion of diamagnetic dust particles in interstellar magnetic fields is studied numerically with several different sets of parameters. Two types of behavior are observed, depending on the value of the critical number $R$, which is a…

星系天体物理 · 物理学 2018-02-21 Renaud Papoular

Dust grains drift through the interstellar medium (ISM) and are aligned with the magnetic field. Here we study the effect of grain alignment and grain motion on grain growth in molecular clouds (MCs). We first discuss the characteristic…

星系天体物理 · 物理学 2022-04-06 Thiem Hoang

We study the stability of charged dust grains orbiting a planet and subject to gravity and the electromagnetic force. Our numerical models cover a broad range of launch distances from the planetary surface to beyond synchronous orbit, and…

地球与行星天体物理 · 物理学 2012-01-18 Daniel Jontof-Hutter , Douglas P. Hamilton

Magnetic fields (B-fields) in galaxies have recently been traced using far-infrared and sub-mm polarimetric observations with SOFIA, JCMT, and ALMA. The main assumption is that dust grains are magnetically aligned with the local B-field in…

星系天体物理 · 物理学 2024-03-01 Enrique Lopez-Rodriguez , Le Ngoc Tram

Aligned non-spherical dust particles polarize starlight passing through the dust cloud. They also emit polarized far infrared and sub-mm radiation. Substantial progress in understanding of grain alignment theory makes the interpretation of…

天体物理学 · 物理学 2007-05-23 A. Lazarian

The interaction between dust grains is an important process in fields as diverse as planetesimal formation or the plasma processing of silicon wafers into computer chips. This interaction depends in large part on the material properties of…

等离子体物理 · 物理学 2009-07-03 Jonathan Perry , Lorin Matthews , Truell Hyde

The interaction between dust grains is an important process in fields as diverse as planetesimal formation or the plasma processing of silicon wafers into computer chips. This interaction depends in large part on the material properties of…

等离子体物理 · 物理学 2015-05-18 Jonathan Perry , Lorin Matthews , Truell Hyde

The deflection of interstellar dust grains in the magnetic field near the heliopause has been investigated based on the assumption that interstellar grains are homogeneous spheres. However, remote observations have shown that interstellar…

等离子体物理 · 物理学 2011-11-02 Qianyu Ma , Lorin Matthews , Victor Land , Truell Hyde

We discuss the rotational excitation of small interstellar grains and the resulting electric dipole radiation from spinning dust. Attention is given to excitation and damping of rotation by: collisions with neutrals; collisions with ions;…

天体物理学 · 物理学 2011-05-05 B. T. Draine , A. Lazarian

We discuss the dynamics of dust grains subjected to uncompensated torques arising from H_2 formation. In particular, we discuss grain dynamics when a grain spins down and goes through a ``crossover''. As first pointed out by Spitzer &…

天体物理学 · 物理学 2009-10-28 A. Lazarian , B. T. Draine

The optical and magnetic properties of dust grains are reviewed, as they relate to the problem of interstellar grain alignment. Grain geometry plays an important role in determining the optical properties, and scattering and absorption of…

天体物理学 · 物理学 2007-05-23 B. T. Draine

We study the radial and vertical stability of dust grains launched with all charge-to-mass ratios at arbitrary distances from rotating planets with complex magnetic fields. We show that the aligned dipole magnetic field model analyzed by…

地球与行星天体物理 · 物理学 2012-06-06 Daniel Jontof-Hutter , Douglas P. Hamilton

This paper provides a quantitative account of a recently introduced mechanism of mechanical alignment of suprathermally rotating grains. These rapidly rotating grains are essentially not susceptible to random torques arising from gas-grain…

天体物理学 · 物理学 2009-10-28 Alex Lazarian , Michael Efroimsky
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