21 Cm Hydrogen-Line Survey Of The Large Magellanic Cloud Ii. Distribution And Motions Of Neutral Hydrogen [PDF]
The 21 cm hydrogen-line data from a survey of the Large Magellanic Oloud with a 14',5 aerial beam have been simplified into distributions of intensities and radial velocities at profile peaks. Fifty-two large HI complexes of mean diameter 575 pc, density I hydrogen atom per cm3, and mass 4 X 106M o have been delineated.
openaire +1 more source
A survey of neutral hydrogen in the Clouds of Magellan has been made using a digital recording system in conjunction with a multichannel receiver and a 21 ft aerial.
M Beard +4 more
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A New High-latitude H i Cloud Complex Entrained in the Northern Fermi Bubble
We report the discovery of 11 high-velocity H i clouds at Galactic latitudes of 25°–30°, likely embedded in the Milky Way’s nuclear wind. The clouds are detected with deep Green Bank Telescope 21 cm observations of a 3 $\mathop{.}\limits^{\unicode{x000b0}
Rongmon Bordoloi +2 more
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Interpretation of the Spatial Power Spectra of Neutral Hydrogen in the Galaxy and in the Small Magellanic Cloud [PDF]
13 pages, 1 figure, to appear in ...
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Early-type galaxies with neutral hydrogen in the Virgo cluster from the ALFALFA survey
We extend our published work on the neutral hydrogen content of early-type galaxies in the Virgo cluster using the catalogue of detected sources from the ALFALFA survey, by showing the 21cm spectra of all the detected galaxies and discussing a deeper ...
PELLEGRINI, SILVIA +4 more
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FAST Observations of Filamentary and Compact H i Structure in the Magellanic Stream IV Field
The Magellanic Stream (MS) is believed to have formed from gas removed from the Large and Small Magellanic Clouds through tidal forces and hydrodynamic interactions with the Milky Way’s gaseous halo.
Yuxin Xiao +5 more
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The significance of hydrogen derivates
Hydrogen and its derivates are expected to play a central role in future, climate-neutral energy systems as secondary energy carrier. This presentation introduces various hydrogen derivates.
Carels, Fabian, Kaltschmitt, Martin
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A large, chemically enriched, neutral gas reservoir in a galaxy at z = 6.782
The physical and chemical characterization of galaxies formed within the first billion years after the Big Bang remains one of the central goals in contemporary astrophysics.
Saccardi A. +25 more
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Revisiting the Vertical Distribution of H i Absorbing Clouds in the Solar Neighborhood
The vertical distribution of cold neutral hydrogen (H i ) clouds is a constraint on models of the structure, dynamics, and hydrostatic balance of the interstellar medium.
Trey V. Wenger +2 more
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Searching for Neutral Hydrogen Escape from the 120 Myr Old Sub-Neptune HIP94235b using HST [PDF]
HIP94235 b, a 120 Myr old sub-Neptune, provides us the unique opportunity to study mass loss at a pivotal stage of the system's evolution: the end of a 100 Myr old phase of intense XUV irradiation.
Rockcliffe, Keighley E. +11 more
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