Results 61 to 70 of about 1,698,518 (186)
On the Existence, Rareness, and Uniqueness of Quenched H i-rich Galaxies in the Local Universe
The Astrophysical JournalUsing data from ALFALFA, xGASS, H i -MaNGA, and the Sloan Digital Sky Survey (SDSS), we identify a sample of 47 “red but H i -rich” (RR) galaxies with near-UV (NUV) − r > 5 and unusually high H i -to-stellar mass ratios. We compare the optical properties
Xiao Li +5 more
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Measurements of Magnetic Fields in Interstellar Clouds of Neutral Hydrogen
The Astrophysical Journal, 1969 A new series of measurements of the Zeeman splitting of 21-cm spectral lines has revealed strong (> 10−5 G) magnetic field effects in several neutral hydrogen clouds in the direction of HII regions. Low limits have been set to the line-of-sight field components in six other regions of space.
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The Astronomical JournalCold neutral hydrogen (H i ) is a crucial precursor for molecular gas formation and can be studied via H i absorption. This study investigates H i absorption in low column density regions of the Small and Large Magellanic Clouds (SMC and LMC) using the ...
Hongxing Chen +20 more
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THE MATHEMATICAL MODELING OF THE PROCESS OF NEUTRALIZATION CLOUDS OF HYDROGEN CYANIDE
Science and Transport Progress, 2008 A computer model to calculate the neutralization of НСN cloud is proposed. The model is based on the numerical integration of the 3-D gradient transport model. The results of numerical experiment are presented.
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The Astrophysical JournalThe presence of dense, neutral hydrogen clouds in the hot, diffuse intragroup and intracluster (IC) medium is an important clue to the physical processes controlling the survival of cold gas and sheds light on cosmological baryon flows in massive halos ...
Avinash Chaturvedi +6 more
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Origin of the Multiphase Interstellar Medium: The Effects of Turbulence and Magnetic Field
The Astrophysical JournalThe interstellar medium (ISM) consists of multiphase gas, including the warm neutral medium (WNM), the unstable neutral medium (UNM), and the cold neutral medium (CNM).
Yue Hu
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Characterizing 3D Magnetic Fields and Turbulence in H I Clouds
The Astrophysical Journal3D Galactic magnetic fields are critical for understanding the interstellar medium, Galactic foreground polarization, and the propagation of ultra-high-energy cosmic rays.
Yue Hu
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Astronomy & AstrophysicsRecent JWST observations of massive galaxies at z > 2 detect blueshifted absorption in Na I D and other resonant absorption lines, indicative of strong gas outflows in the neutral phase.
Moretti Lorenzo +7 more
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On The Origin Of Neutral Hydrogen Clouds In Nearby Galaxy Groups: The Role Of Galaxy Interactions
, 2010 This thesis addresses the origin of the High Velocity Clouds (HVCs) observed around the Milky Way and other nearby galaxies. Such clouds are likely created through a combination of galactic fountains, galaxy interactions, dark matter substructure, and ...
Chynoweth, Katie Mae
core
, 2022 Publisher Copyright: © 2022 Proceedings of WHEC 2022 - 23rd World Hydrogen Energy Conference: Bridging Continents by H2. All rights reserved.This work addresses the potential of hydrogen injection into the transmission high pressure natural gas grid as ...
Madina, Virginia +5 more
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