Results 61 to 70 of about 345 (143)

Influence of Density Distribution on Synchrotron Polarization Dispersion in Magnetized Interstellar Medium

open access: yesThe Astrophysical Journal
Faraday rotation measure (RM) synthesis is a well-known approach originated in B. J. Burn and later developed by M. A. Brentjens & A. G. de Bruyn for studying magnetic fields.
Ya-Wen Xiao   +3 more
doaj   +1 more source

The Effects of Cosmic-Ray Protons on Galactic Nonthermal Filaments

open access: yesThe Astrophysical Journal
The Galactic center (GC) contains a collection of filaments that are typically tens of parsecs in length, illuminated by synchrotron radiation from cosmic rays (CRs). The origin of these nonthermal filaments (NTFs) is unclear.
Mohan Richter-Addo   +4 more
doaj   +1 more source

Robust magnetic field estimates in star-forming galaxies with the equipartition formula in the absence of equipartition

open access: yesAstronomy & Astrophysics
The equipartition model is widely used to estimate magnetic field strength from synchrotron intensity in radio galaxies, yet the validity of its underlying assumptions remains uncertain.
Sandy Chiu H.-H.   +4 more
doaj   +1 more source

Recovering 3D Magnetic Turbulence from Single-frequency Faraday Screens

open access: yesThe Astrophysical Journal
Statistics of polarized synchrotron radiation carry information about the properties of the underlying turbulence. We consider a setup in which synchrotron radiation is emitted in a distant volume and then passes through a turbulent screen that induces ...
A. Melnichenka, A. Lazarian, D. Pogosyan
doaj   +1 more source

87th Annual Meeting of the Meteoritical Society 2025: Abstracts

open access: yes
Meteoritics &Planetary Science, Volume 60, Issue S1, Page 30-350, August 2025.
wiley   +1 more source

First Detection of Circular Polarization in Radio Continuum Toward a Massive Protostar

open access: yesThe Astrophysical Journal Letters
Polarization measurements provide strong constraints on magnetic fields in star-forming systems. While magnetic field estimates of a few kG have been obtained near the surfaces of low-mass protostars, there are no analogous measurements in the immediate ...
A. G. Cheriyan   +6 more
doaj   +1 more source

Particle Acceleration and Depolarization in the Protostellar Jet Knots HH 80 and HH 81

open access: yesThe Astrophysical Journal
Linearly polarized emission is a powerful tracer of magnetic field geometry and particle acceleration in protostellar jets. We present a polarimetric study of the Herbig–Haro (HH) objects HH 80 and HH 81, where nonthermal emission has been confirmed ...
A. G. Cheriyan   +6 more
doaj   +1 more source

Spatially resolved interstellar dust properties in the face-on spiral galaxy M 99 as observed by NIKA2

open access: yesAstronomy & Astrophysics
Context. Large dust grains in thermal equilibrium dominate the far-infrared emission of star-forming galaxies and substantially contribute to their millimetre continuum. Constraining dust properties in this regime is challenging due to contamination from
Pantoni L.   +64 more
doaj   +1 more source

The cosmic ray ionization and γ-ray budgets of star-forming galaxies. [PDF]

open access: yesMon Not R Astron Soc, 2023
Krumholz MR, Crocker RM, Offner SSR.
europepmc   +1 more source

The Radio and Microwave Sky as Seen by Juno on its Mission to Jupiter

open access: yesThe Astrophysical Journal
We present six nearly full-sky maps made from data taken by radiometers on the Juno satellite during its 5 yr flight to Jupiter. The maps represent integrated emission over ∼4% passbands spaced approximately in octaves between 600 MHz and 21.9 GHz.
C. J. Anderson   +6 more
doaj   +1 more source

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