Results 141 to 150 of about 143,809 (350)
Velocity Structure and Molecular Formation in the Polaris Molecular Cloud
We present a wide-field $(60^{\prime} \times 30^{\prime} )$ study of a dense region within the Polaris Flare using ^12 CO, ^13 CO, and C ^18 O ( J = 1–0) observations at 15″ resolution, obtained with the Nobeyama 45 m Radio Telescope.
Tomomi Shimoikura +3 more
doaj +1 more source
Dust Emission from the Perseus Molecular Cloud [PDF]
S. Schnée +7 more
openalex +1 more source
Cosmic Rays and Molecular Clouds [PDF]
To appear in the proceedings of the San Cugat Forum on Astrophysics 2012, 27 pages, 10 ...
openaire +3 more sources
Melt Grafting of Geometry‐Tailored Voltage Stabilizers for High‐Performance Polypropylene Insulation
A scalable one‐step melt grafting strategy is developed to enhance the dielectric properties of isotactic polypropylene by covalently incorporating thermally stable aromatic voltage stabilizers. This solvent‐free approach improves volume resistivity and DC breakdown strength through deep trap formation and charge localization, offering a sustainable ...
Nazirul Mubin bin Normansah +9 more
wiley +1 more source
Astronomers have used observations of the Galactic gas and dust via infrared, microwave, and radio to study molecular clouds in extreme environments such as the Galactic center.
Samantha W. Brunker +7 more
doaj +1 more source
Cloud-cloud collision as drivers of the chemical complexity in Galactic Centre molecular clouds. [PDF]
Zeng S +8 more
europepmc +1 more source
Are Ultraluminous X‐Ray Sources Intermediate‐Mass Black Holes Accreting from Molecular Clouds? [PDF]
Julian H. Krolik
openalex +1 more source
Advances in Stimuli‐Responsive Organic Materials and Polymers toward Intelligent CO2 Capture
Schematic illustration of the relationship between different stimuli and stimuli‐responsive organic materials and polymers for carbon dioxide (CO2) capture. Main stimuli include redox, pH, magnetism, temperature, light, and pressure. Furthermore, multi‐responsive materials, due to their high adaptability and scalability in complex environments, are ...
Jian Zhou +2 more
wiley +1 more source
Deep interferometric observations of CO and dust continuum emission are obtained with the Submillimeter Array at 230 GHz to investigate the physical nature of the giant molecular cloud (GMC) population in the Andromeda galaxy (M31).
Charles J. Lada +3 more
doaj +1 more source
The Thermodynamics of Molecular Cloud Fragmentation: Star Formation Under Non-Milky Way Conditions [PDF]
S. Hocuk, M. Spaans
openalex +1 more source

