In addition to the anisotropic expansion of I - fronts into a filament, B - fields are expected to introduce an additional anisotropic press... ▽ More The influence of magnetic fields (B - fields) in the formation and evolution of bipolar bubbles, due to the expanding ionization fronts (I - fronts) driven by the Hii regions that are formed and embedded
in filamentary molecular clouds, has not been well - studied yet.
Abstract: The influence of magnetic fields (B - fields) in the formation and evolution of bipolar bubbles, due to the expanding ionization fronts (I - fronts) driven by the Hii regions that are formed and embedded
in filamentary molecular clouds, has not been well - studied yet.
Not exact matches
Williams, of Cardiff University, explains: «We've known for some time that dusty,
filamentary cloud structures are ubiquitous
in the Milky Way's interstellar medium.
Supercomputer simulations model how galaxies and galactic clusters grow
in long
filamentary structures known as the cosmic web.
The MAMMOTH - 1 nebula appears to have a
filamentary structure that aligns with the galaxy distribution
in the large - scale structure of the protocluster, supporting the idea that ELANs are illuminated segments of the cosmic web, Cai said.
The
filamentary structure
in SSA22 could be called a proto - Great Wall.
This dark matter
filamentary structure is thought to be a progenitor of large scale structures
in the Universe.
One of the best known examples of large scale structure
in the modern Universe is the cosmic Great Wall, a gigantic
filamentary structure spanning over 500 million light - years.
In the final sequence, the viewer enters an immersive exploration of the
filamentary structure of the local universe, navigating inside the filaments and visiting the major nodes such as the Great Attractor.
The image shows a fine web of
filamentary «bicycle - spoke» features embedded
in the colorful red and blue ring of gas.
We have clearly detected FIR dust emission extended
in the halo of the galaxy; there are two
filamentary emission structures extending from the galactic disk up to 9 kpc
in the northern and 6 kpc
in the northwestern direct... ▽ More We present new far - infrared (FIR) images of the edge - on starburst galaxy NGC253 obtained with the Far - Infrared Surveyor (FIS) onboard AKARI at wavelengths of 90 um and 140 um.
Galaxies are actually believed to draw
in gas that resides along
filamentary strings.
«I wonder if we can indeed use this technique to see the emission of
filamentary gas
in the cosmic web.
The gravitational interaction has also resulted
in the formation of
filamentary structures
in the group.