Results 101 to 110 of about 43,858 (281)
Strottner–Drechsler–Sainty Object 1 (SDSO1) is a faint [O iii ] emission nebula spanning 1 $\mathop{.}\limits^{^\circ }5$ , discovered southeast of M31.
Tiantian Liang +18 more
doaj +1 more source
We present high-spatial resolution 21-cm HI VLA observations of the radio galaxy 3C305 (z=0.041). These new high-resolution data show that the ~1000 km/s broad HI absorption, earlier detected in low-resolution WSRT observations, is occurring against the ...
B. Emonts +25 more
core +2 more sources
Comparative Insights and Overlooked Factors of Interphase Chemistry in Alkali Metal‐Ion Batteries
This review presents a comparative analysis of Li‐, Na‐, and K‐ion batteries, focusing on the critical role of electrode–electrolyte interphases. It especially highlights overlooked aspects such as SEI/CEI misconceptions, binder effects, and self‐discharge relevance, emphasizing the limitations of current understanding and offering strategies for ...
Changhee Lee +3 more
wiley +1 more source
Multiscale perspectives on how excess charges in soft lead halide perovskites induce operational instability in photovoltaic devices are presented. Localized carriers formed under thermodynamic non‐equilibrium states modify atomistic interactions and drive lattice distortions, accelerating device degradation.
Joo‐Hong Lee +6 more
wiley +1 more source
A New Look at the Kinematics of Neutral Hydrogen in the Small Magellanic Cloud
We have used the latest HI observations of the Small Magellanic Cloud (SMC), obtained with the Australia Telescope Compact Array and the Parkes telescope, to re-examine the kinematics of this dwarf, irregular galaxy. A large velocity gradient is found in the HI velocity field with a significant symmetry in iso-velocity contours, suggestive of a ...
Stanimirovic, S. +2 more
openaire +2 more sources
Metallicity Mapping of the Ionized Diffuse Gas at the Milky Way Disk–Halo Interface
Metals in the diffuse, ionized gas at the boundary between the Milky Way’s interstellar medium (ISM) and circumgalactic medium, known as the disk–halo interface (DHI), are valuable tracers of the feedback processes that drive the Galactic fountain ...
Bo-Eun Choi +7 more
doaj +1 more source
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 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
doaj +1 more source
Compact Galactic Neutral Hydrogen Clouds in the GALFA-HI Survey
The more sensitive the observations, the more complex the gas in our Galaxy appears. Since the detection of neutral hydrogen in 1951, each new survey has revealed new structure. Using the GALFA-HI survey, we have discovered five populations of compact neutral hydrogen clouds.
openaire +2 more sources
Neutral hydrogen absorption in the quasar 3C 268.4 - Possible evidence for galactic halo clouds
We have detected neutral hydrogen absorption at 21 cm wavelength in the quasar-galaxy pair 3C 268.4/NGC 4138. The absorption spectrum exhibits two features which are separated by 65 and -120 km s/sup -1/, respectively, from the center velocity of 880 km s/sup -1/ of the neutral hydrogen emission profile from NGC 4138. The line of sight of the quasar 3C
A. D. Haschick, P. C. Crane, W. A. Baan
openaire +1 more source

