Results 71 to 80 of about 135,058 (169)
A multiscale dynamical mass-assembly scenario, where stars form through multiscale fragmentation and hierarchical gas infall from clouds to filaments, clumps, and cores, has been proposed for high-mass star formation, but the precise observational ...
Chengzhi Meng +10 more
doaj +1 more source
Interstellar filaments and the statistics of galactic HI
This paper presents a statistical explanation of filament formation in the galactic atomic hydrogen. We claim that even in the absence of dynamical factors the Gaussian field corresponding to the measured values of the spectrum of random density should ...
A. Lazarian +2 more
core
Flexible polymer-induced condensation and bundle formation of DNA and F-actin filaments [PDF]
A simple semi-empirical theory is developed for the ionic strength dependence of the flexible polymer-induced condensation of semiflexible polyelectrolytes such as DNA and F-actin filaments.
Vries, R., de
core
Bubbles and holes in the interstellar medium
Studies of the HI in nearby galaxies now clearly begin to show the effects of star formation on the interstellar medium. Holes, filaments, expanding motions and other anomalous velocity signatures are clearly apparent in sensitive observations of the HI ...
vanderHulst, JM +1 more
core +1 more source
Observations of the interstellar medium (ISM) at far-infrared and submillimeter wavelengths reveal a complex filamentary structure of dust and gas, which plays a pivotal role in both low- and high-mass star formation.
Shivam Kumaran +5 more
doaj +1 more source
We report 850 μ m continuum polarization observations toward the filamentary high-mass star-forming region NGC 2264, taken as part of the B -fields In STar forming Regions Observations large program on the James Clerk Maxwell Telescope. These data reveal
Jia-Wei Wang +156 more
doaj +1 more source
Cosmic-Ray Feedback on Bistable Interstellar Medium Turbulence
While cosmic rays ( E ≳ 1 GeV) are well coupled to a galaxy’s interstellar medium (ISM) at scales of L > 100 pc, adjusting stratification and driving outflows, their impact on small scales is less clear.
Roark Habegger +3 more
doaj +1 more source
Cluster Formation in a Filamentary Cloud: The Case of the Stellar Cluster NGC 2316
We present a multiwavelength analysis of the star cluster NGC 2316 and its surroundings. We estimated the physical parameters of the NGC 2316 cluster, including its shape (elongated), size ( R _cluster = 0.4 pc), distance (1.3 ± 0.3 kpc), and minimum ...
Saurabh Sharma +9 more
doaj +1 more source
Dust in and Around the Heliosphere and Astrospheres. [PDF]
Sterken VJ +9 more
europepmc +1 more source
Internal 1000 au Scale Structures of the R CrA Cluster-forming Cloud. I. Filamentary Structures
We report Atacama Large Millimeter/submillimeter Array/Atacama Compact Array observations of a high-density region of the Corona Australis cloud forming a young star cluster, and the results of resolving internal structures. In addition to embedded Class
Kengo Tachihara +19 more
doaj +1 more source

