Results 41 to 50 of about 3,801,891 (296)
CO Structures with Narrow Lines in Nearby Quiescent Regions
Using CO data from Phase I of the Milky Way Imaging Scroll Painting survey, we present a systematic study of molecular structures with narrow lines.
Ruilin Xia +15 more
doaj +1 more source
Are Supernovae Responsible for the Gamma Ray Spectrum from the Galactic Center?
We discuss the supernova remnants distribution as a function of the galactic longitude and compare their positions to that of the detected TeV gamma ray sources. A large fraction of these sources either coincide or a close by known supernova remnants. If
Todor Stanev
doaj +1 more source
Enhancing Low‐Temperature Performance of Sodium‐Ion Batteries via Anion‐Solvent Interactions
DOL is introduced into electrolytes as a co‐solvent, increasing slat solubility, ion conductivity, and the de‐solvent process, and forming an anion‐rich solvent shell due to its high interaction with anion. With the above virtues, the batteries using this electrolyte exhibit excellent cycling stability at low temperatures. Abstract Sodium‐ion batteries
Cheng Zheng +7 more
wiley +1 more source
Comparing the Locations of Supernovae to CO (2–1) Emission in Their Host Galaxies
We measure the molecular gas environment near recent (
Ness Mayker Chen +21 more
doaj +1 more source
Observational Constraints for Modeling Diffuse Molecular Clouds [PDF]
AbstractGround-based and space-borne observations of diffuse molecular clouds suggest a number of areas where further improvements to modeling efforts is warranted. I will highlight those that have the widest applicability. The range in CO fractionation caused by selective isotope photodissociation, in particular the large 12C16O/13C16O ratios observed
openaire +1 more source
Diffusive versus Free-streaming Cosmic-Ray Transport in Molecular Clouds [PDF]
Abstract Understanding the cosmic-ray (CR) ionization rate is crucial in order to simulate the dynamics of molecular clouds, and interpret the chemical species observed in these objects. Calculating the CR ionization rate requires both accurate knowledge of the spectrum of MeV to GeV protons at the edge of the cloud as well as a model ...
Kedron Silsbee, Alexei V. Ivlev
openaire +3 more sources
Mutual influence of supernovae and molecular clouds [PDF]
International audienceContext. Molecular clouds are known to be turbulent and strongly affected by stellar feedback. Moreover, stellar feedback is believed to drive turbulence at large scales in galaxies.Aims.
Olivier Iffrig +3 more
core +1 more source
Advances in Sustainable and Wearable Textile Based Soft Robotics
This Review examines advances in wearable textile‐based soft robotics, focusing on sustainable materials, integrated sensing, and scalable actuation. It discusses manufacturing and system integration across healthcare, assistive robotics, prosthetics, and human–machine interfaces, and highlights key challenges in circular design, including life‐cycle ...
Zahir Abbas +6 more
wiley +1 more source
We use ^12 CO ( J = 1–0) data from the MWISP survey to investigate turbulence in a ∼kiloparsec-scale segment of the Local Arm. By slicing the position–position–velocity cube into narrow layers that follow the Galactic-rotation trend in the L – V diagram,
Yuehui Ma +7 more
doaj +1 more source
Interstellar shocks and molecular CH/+/ in diffuse clouds
The influence of shocks on the abundances of molecules in diffuse interstellar clouds is investigated with special emphasis on molecular CH/sup +/. Idealized shocks with plausible parameters are found to produce column densities for CH/sup +/ in the hot, postshock gas which are comparable with measured values in interstellar clouds (up to about 10/sup ...
M. Elitzur, W. D. Watson
openaire +1 more source

