Results 21 to 30 of about 4,796,716 (321)
THE CALIFORNIA MOLECULAR CLOUD [PDF]
Accepted for publication in the ApJ. This submission has low resolution figures. Preprint with full resolution figures can be found at http://www.cfa.harvard.edu/~clada/pubs_html/California ...
C. J. Lada, M. Lombardi, J. F. Alves
openaire +2 more sources
Background Exposure to air pollutants is one of the major environmental health risks faced by populations globally. Information about inhaled particle deposition dose is crucial in establishing the dose–response function for assessing health-related ...
Leizel Madueño +5 more
doaj +1 more source
Molecular line signatures of cloud–cloud collisions [PDF]
ABSTRACT Collisions between interstellar gas clouds are potentially an important mechanism for triggering star formation. This is because they are able to rapidly generate large masses of dense gas. Observationally, cloud collisions are often identified in position–velocity (PV) space through bridging features between intensity peaks ...
Priestley, F. D., Whitworth, A. P.
openaire +3 more sources
The Role of Magnetic Field in Molecular Cloud Formation and Evolution [PDF]
We review the role that magnetic field may have on the formation and evolution of molecular clouds. After a brief presentation and main assumptions leading to ideal MHD equations, their most important correction, namely the ion-neutral drift is described.
P. Hennebelle, S. Inutsuka
semanticscholar +1 more source
Multi-line characterization of whole molecular clouds using stratified random sampling [PDF]
We have developed a new technique to characterize the multi-line emission from molecular clouds using statistical sampling. Our method uses available extinction maps to select a relatively small sample of cloud positions that cover the full range of ...
Tafalla Mario +2 more
doaj +1 more source
Mapping Distances across the Perseus Molecular Cloud Using CO Observations, Stellar Photometry, and Gaia DR2 Parallax Measurements [PDF]
We present a new technique to determine distances to major star-forming regions across the Perseus Molecular Cloud, using a combination of stellar photometry, astrometric data, and 12CO spectral-line maps. Incorporating the Gaia DR2 parallax measurements
C. Zucker +6 more
semanticscholar +1 more source
The interaction between a molecular cloud and an external agent (e.g., a supernova remnant, plasma jet, radiation, or another cloud) is a common phenomenon throughout the Universe and can significantly change the star formation rate within a galaxy. This
B. Albertazzi +12 more
doaj +1 more source
The LEGO Large Program: Constraining the Physics of Line Emission in Galaxy Observations [PDF]
The IRAM Large Program LEGO studies molecular clouds in the Milky Way to constrain the physics controlling molecular line emission in galaxies. This is done by imaging two dozen clouds with setups that provide continuous spectral coverage of about 85–115
Kauffmann Jens, Barnes Ashley
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Star cluster formation in a turbulent molecular cloud self-regulated by photoionization feedback [PDF]
Most stars in the Galaxy are believed to be formed within star clusters from collapsing molecular clouds. However, the complete process of star formation, from the parent cloud to a gas-free star cluster, is still poorly understood.
E. Gavagnin +3 more
semanticscholar +1 more source
Making it Rain: Cloud-Based Molecular Simulations for Everyone
We present a user-friendly front-end for running molecular dynamics (MD) simulations using the OpenMM toolkit on the Google Colab framework. Our goals are (1) to highlight the usage of a cloud-computing scheme for educational purposes for a hands-on ...
P. Arantes +3 more
semanticscholar +1 more source

