Results 11 to 20 of about 103,451 (210)
The Turbulent Interstellar Medium [PDF]
An overview is presented of the main properties of the interstellar medium. Evidence is summarized that the interstellar medium is highly turbulent, driven on different length scales by various energetic processes.
Andreas Burkert +73 more
core +5 more sources
Interstellar Polarization Survey. II. General Interstellar Medium
Magnetic fields permeate the entire Galaxy and are essential to, for example, the regulation of several stages of the star formation process and cosmic-ray transportation.
M. J. F. Versteeg +6 more
doaj +4 more sources
Observations of the Outer Heliosphere, Heliosheath, and Interstellar Medium [PDF]
John D Richardson +2 more
exaly +2 more sources
An Innovative Approach for the Generation of Species of the Interstellar Medium [PDF]
Lucie Kolesniková +2 more
exaly +2 more sources
Measurement of MHD Turbulence Properties by Synchrotron Radiation Techniques
It is well known that magnetohydrodynamic (MHD) turbulence is ubiquitous in astrophysical environments. The correct understanding of the fundamental properties of MHD turbulence is a pre-requisite for revealing many key astrophysical processes.
Jian-Fu Zhang +2 more
doaj +1 more source
Mass Distribution for Single-lined Hot Subdwarf Stars in LAMOST
Masses for 664 single-lined hot subdwarf stars identified in LAMOST were calculated by comparing synthetic fluxes from spectral energy distribution with observed fluxes from a Virtual Observatory service.
Zhenxin Lei +6 more
doaj +1 more source
Hot Subdwarf Stars Identified in LAMOST DR8 with Single-lined and Composite Spectra
A total of 222 hot subdwarf stars were identified with LAMOST DR8 spectra, among which 131 stars show composite spectra and have been decomposed, while 91 stars present single-lined spectra.
Zhenxin Lei +8 more
doaj +1 more source
Magnetic-reconnection-driven Turbulence and Turbulent Reconnection Acceleration
This paper employs an MHD-PIC method to perform numerical simulations of magnetic-reconnection-driven turbulence and turbulent reconnection acceleration of particles.
Shi-Min Liang +3 more
doaj +1 more source
Voyager Observations of Electron Densities in the Very Local Interstellar Medium
The two Voyager spacecraft have now been immersed in the very local interstellar medium for several years. Both spacecraft carry a plasma wave instrument capable of detecting plasma waves that yield electron density through the determination of the ...
W. S. Kurth +4 more
doaj +1 more source
Rubidium in the Interstellar Medium [PDF]
We present observations of interstellar rubidium toward o Per, zeta Per, AE Aur, HD 147889, chi Oph, zeta Oph, and 20 Aql. Theory suggests that stable 85Rb and long-lived 87Rb are produced predominantly by high-mass stars, through a combination of the ...
Abia +28 more
core +2 more sources

