Results 21 to 30 of about 832,537 (179)
Metastable Nanosized Diamond Formation from Fluid Systems [PDF]
The model of nanosized diamond particles formation at metastable P-T parameters from fluid is presented. It explains the specific of CVD diamond synthesis gases mixtures and hydrothermal growth of diamond at low P-T parameters as well as it explains the ...
Sergei Simakov
core +1 more source
A photon transport problem with a time-dependent point source [PDF]
We consider a time-dependent problem of photon transport in an interstellar cloud with a point photon source modeled by a Dirac δ functional. The existence of a unique distributional solution to this problem is established by using the theory of ...
McBride, A.C. +2 more
core +3 more sources
Heating of the low-latitude solar wind by dissipation of turbulent magnetic fluctuations [PDF]
We test a theory presented previously to account for the turbulent transport of magnetic fluctuation energy in the solar wind and the related dissipation and heating of the ambient ion population. This theory accounts for the injection of magnetic energy
Matthaeus, William H. +5 more
core +1 more source
Investigating the IBEX Ribbon Structure a Solar Cycle Apart
A “Ribbon” of enhanced energetic neutral atom (ENA) emissions was discovered by the Interstellar Boundary Explorer in 2009, redefining our understanding of the heliosphere boundaries and the physical processes occurring at the interstellar interface. The
M. A. Dayeh +3 more
doaj +1 more source
Research on the interstellar medium and its interaction with the solar system constitutes a significant topic in planetary physics. As the Sun traverses the local interstellar cloud, interstellar neutrals penetrate the heliosphere, forming the ...
JiaLing Lyu +3 more
doaj +1 more source
Properties of Star Formation of the Large Magellanic Cloud As Probed by Young Stellar Objects
We perform a systematic study of the evolutionary stages and stellar masses of young stellar objects (YSOs) in the Large Magellanic Cloud (LMC) to investigate the properties of star formation in the galaxy. There are 4825 sources in our YSO sample, which
Takuma Kokusho +4 more
doaj +1 more source
The reaction between the methanol radical cation and sulfur dioxide is remarkably fast and forms several ionic and neutral products (HOSOH+, CH2OSO+, CH2OH+, CH2O, H2O, HSO2). The chemistry goes beyond simple proton or hydrogen transfer, revealing a close interaction between the two species, relevant to atmospheric and astrochemical environments where ...
Mauro Satta +3 more
wiley +1 more source
The formation of molecular hydrogen in the interstellar medium [PDF]
H2 is the most abundant molecule in the interstellar medium and forms on the surface of interstellar dust grains. Laboratory studies have been conducted of HD formation on a dust grain analogue, which is a highly-oriented pyrolytic graphite surface ...
Islam, F.
core
Based on the slopes between DESI g , r and Infrared Astronomical Satellite (IRAS) 100 μ m intensities, specifically k _g and k _r , we have constructed a substantial sample of Galactic cirri. This sample covers 561.25 deg ^2 at high Galactic latitudes (∣
Yunning Zhao +4 more
doaj +1 more source
Optical Radiation Pressure: Resonant Mechanical Excitation of Thin Films
The modulation of a laser beam generates a modulated radiation pressure force acting on a thin film. A resonant response is observed, leading to a net average thinning of the film. ABSTRACT Optical radiation pressure was directly observed for the first time more than a century ago.
Janine Emile, Olivier Emile
wiley +1 more source

