Results 261 to 270 of about 43,858 (281)
Some of the next articles are maybe not open access.

Further Measurements of Magnetic Fields in Interstellar Clouds of Neutral Hydrogen

Nature, 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.
openaire   +3 more sources

The Leo Intergalactic Neutral Hydrogen Cloud

1986
The current status of the neutral hydrogen λ21 cm radio observations of the intergalactic cloud in Leo are described. These include both HI observations at Arecibo with an angular resolution of ∼3 arc min, and VLA D-array observations with an effective resolution of 45 arc sec.
Yervant Terzian   +2 more
openaire   +1 more source

The distance to two neutral hydrogen clouds

The Astrophysical Journal, 1996
A lower limit to the distance of the high-velocity cloud (HVC) complex A of 4 kpc (z > 3 kpc) is derived. The HVC is detected toward the Seyfert galaxy Mrk 106 in Mg II lambda lambda 2796, 2803 absorption spectra taken with Hubble Space Telescope (HST) proving that Mg+ is present in the cloud. It is not detected in the Mg II spectra of two stars, PG
Wakker, B   +7 more
openaire   +1 more source

Cooling of Interstellar Clouds of Neutral Hydrogen and the Abundance of Molecular Hydrogen

Publications of the Astronomical Society of Japan, 1968
Abstract The structure of the radiative cooling layer behind the shock front due to interstellar cloud-collision is calculated for a collision velocity of Mach number 20 (~ 16 km/sec). The magnetic field is assumed to be 0 or 10–5 gauss parallel to the shock front. The cooling mechanisms involved are the collision of H atoms with O atoms,
openaire   +1 more source

Properties of the Neutral Hydrogen in the Magellanic Clouds

1971
The first low-resolution survey of the neutral hydrogen in the Clouds (Kerr et al., 1954) showed the existence of large Hi envelopes around both Clouds and an unexpectedly large gas content for the Small Cloud. The second survey (Hindman et al., 1963) was also carried out with a small telescope but a better receiver was used; this study confirmed the ...
openaire   +1 more source

Acoustically‐Induced Water Frustration for Enhanced Hydrogen Evolution Reaction in Neutral Electrolytes

Advanced Energy Materials, 2023
Yemima Ehrnst   +2 more
exaly  

Catalytic self-transfer hydrogenolysis of lignin with endogenous hydrogen: road to the carbon-neutral future

Chemical Society Reviews, 2022
Xiaojun Shen, Chaofeng Zhang, Buxing Han
exaly  

Multi-site electrocatalysts for hydrogen evolution in neutral media by destabilization of water molecules

Nature Energy, 2018
Cao-Thang Dinh   +2 more
exaly  

Home - About - Disclaimer - Privacy