Results 1 to 10 of about 13,169 (193)
Herschel observation has recently revealed that interstellar molecular clouds consist of many filaments. Polarization observations in optical and infrared wavelengths indicate that the magnetic field often runs perpendicular to the filament.
Tomisaka, Kohji
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We present the results of molecular line observations toward the W40 and Serpens South regions of the Aquila molecular cloud complex, conducted as part of the Taeduk Radio Astronomy Observatory survey of Filaments, the Universal Nursery of Stars project ...
Satyajeet Moharana +11 more
doaj +1 more source
We present an analysis of polarized dust emission at 850 μ m for a parsec-long filament in the northern part of the Orion B molecular cloud. The region was observed by the James Clerk Maxwell Telescope SCUBA-2/POL-2 polarimeter.
Kshitiz K. Mallick +7 more
doaj +1 more source
High-resolution surveys reveal that the interstellar medium in the Milky Way and nearby galaxies consists of interlinked hierarchies of filamentary structure and superbubbles extending from galactic to subparsec scales.
Rachel Pillsworth +3 more
doaj +1 more source
Simulations of cosmic ray propagation. [PDF]
Hanasz M, Strong AW, Girichidis P.
europepmc +1 more source
The past two decades have seen extensive surveys of the far-infrared to submillimeter continuum emission in the plane of our Galaxy. We line out prospects for the coming decade for corresponding molecular and atomic line surveys which are needed to fully
Beuther, Henrik +13 more
core
Dense filaments are believed to be representative of the initial conditions of star formation in molecular clouds. We have used the MIRI instrument on JWST to image the massive filament NGC 6334M at d ∼ 1.3 kpc with unprecedented resolution and dynamic ...
Philippe André +6 more
doaj +1 more source
The supernova remnant SN 1006 as a Galactic particle accelerator. [PDF]
Giuffrida R +8 more
europepmc +1 more source
A Catalog of Filaments in the Central Molecular Zone
We present a catalog of 1.28 GHz radio filaments observed by MeerKAT over the innermost 200 pc of the Galaxy (roughly ±1 $\mathop{.}\limits^{\unicode{x000b0}}$ 5), which includes the central molecular zone.
Richard G. Arendt +2 more
doaj +1 more source
Cosmic ray feedback in galaxies and galaxy clusters: A pedagogical introduction and a topical review of the acceleration, transport, observables, and dynamical impact of cosmic rays. [PDF]
Ruszkowski M, Pfrommer C.
europepmc +1 more source

