Results 51 to 60 of about 4,624,977 (307)
The Astrophysical JournalThe recently discovered Eos molecular cloud is a CO-dark, low-density cloud located at a distance of approximately 94 pc from the Sun which does not appear to have formed stars at any point in its history.
Janik Karoly +5 more
doaj +1 more source
Molecular cloud dispersal traced by the ionized carbon 158 μm line
Astronomy & AstrophysicsFeedback from massive stars in the form of radiation and winds impacts the associated host molecular cloud. Not only can feedback compress gas and trigger the formation of dense cores that eventually collapse into new stars, it can also disperse cloud ...
Bonne L. +16 more
doaj +1 more source
Filaments in the Lupus molecular clouds [PDF]
Monthly Notices of the Royal Astronomical Society, 2015 We have studied the filaments extracted from the column density maps of the nearby Lupus 1, 3, and 4 molecular clouds, derived from photometric maps observed with the Herschel satellite. Filaments in the Lupus clouds have quite low column densities, with a median value of $\sim$1.5$\times$10$^{21}$ cm$^{-2}$ and most have masses per unit length lower ...
Benedettini, M. +21 more
openaire +8 more sources
Saint Cloud Reporter [Spring 1969] [PDF]
, 1969 Saint Cloud Reporter, Spring 1969https://repository.stcloudstate.edu/magazines/1121/thumbnail ...
St. Cloud State University
core
Correlated Charge Transport in an Organic Coulomb Glass
Advanced Materials, EarlyView.ABSTRACT Advances in the development of organic field‐effect transistors (OFETs), electrically gated organic semiconductors (EGOFETs), and organic electrochemical transistors (OECTs) allow for the operation of these devices at very high charge‐carrier densities, where Coulomb interactions between carriers can be expected to become significant.
Magdalena Sophie Dörfler +3 more
wiley +1 more source
The Astrophysical Birth Environment of the Solar System Inferred from Cometary Noble Gases
The Astrophysical JournalThe stellar sources that contributed to the chemical and isotopic composition of the solar system, their mixing in the Galactic environment, and the evolution and longevity of the molecular cloud from which our solar system formed can be probed with ...
William S. Cassata +5 more
doaj +1 more source
A Complete HCN Survey of the Perseus Molecular Cloud
The Astrophysical Journal, 2023 We present a survey of the Perseus molecular cloud in the J = 1 → 0 transition of HCN, a widely used tracer of dense molecular gas. The survey was conducted with the CfA 1.2 m telescope, which at 89 GHz has a beamwidth of 11′ and a spectral resolution of
T. M. Dame, Charles J. Lada
doaj +1 more source
Saint Cloud Reporter [Winter 1967] [PDF]
, 1967 Saint Cloud Reporter, Winter 1967https://repository.stcloudstate.edu/magazines/1117/thumbnail ...
St. Cloud State University
core
Organic Materials of Tomorrow: Horizons of Artificial Intelligence
Advanced Materials, EarlyView.This review examines machine learning techniques accelerating the discovery of organic semiconductors by linking molecular structure to properties. Key methods include graph neural networks, generative models, and active learning. Applications to organic photovoltaics demonstrate practical impact.
Harold Mena +3 more
wiley +1 more source
The approach to collapse of molecular clouds [PDF]
Monthly Notices of the Royal Astronomical Society, 2009 The dense molecular cloud cores that form stars, like other self-gravitating objects, undergo bulk oscillations. Just at the point of gravitational instability, their fundamental oscillation mode has zero frequency. We study, using perturbation theory, the evolution of a spherical cloud that possesses such a frozen mode.
Stahler, Steven W., Yen, Jeffrey J.
openaire +2 more sources