The Evolution of the Star-Forming Interstellar Medium Across Cosmic Time [PDF]
Over the past decade increasingly robust estimates of the dense molecular gas content in galaxy populations between redshift 0 and the peak of cosmic galaxy/star formation from redshift 1-3 have become available. This rapid progress has been possible due
L. Tacconi, R. Genzel, A. Sternberg
semanticscholar +1 more source
A non-energetic mechanism for glycine formation in the interstellar medium [PDF]
The detection of the amino acid glycine and its amine precursor methylamine on the comet 67P/Churyumov-Gerasimenko by the Rosetta mission provides strong evidence for a cosmic origin of amino acids on Earth.
S. Ioppolo+10 more
semanticscholar +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
Detection of the aromatic molecule benzonitrile (c-C6H5CN) in the interstellar medium [PDF]
A specific interstellar aromatic molecule Aromatic molecules such as polycyclic aromatic hydrocarbons (PAHs) are known to exist in the interstellar medium owing to their characteristic infrared emission features.
B. McGuire+6 more
semanticscholar +1 more source
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
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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
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Magnetic Turbulence Spectra and Intermittency in the Heliosheath and in the Local Interstellar Medium [PDF]
The understanding of inertial-scale dynamics in the heliosheath is not yet thorough. Magnetic field fluctuations across the inner heliosheath (IHS) and the local interstellar medium (LISM) are here considered to provide accurate and highly resolved ...
F. Fraternale+3 more
semanticscholar +1 more source
Determination of interstellar pickup ion distributions in the solar wind with SOHO and Cluster [PDF]
Over the last 10 years, the experimental basis for the study of the local interstellar medium has been substantially enhanced by the direct detection of interstellar pickup ions and of interstellar neutral helium within the heliosphere.
E. Möbius+3 more
doaj +1 more source