Modeling the Impact of Moderate External UV Irradiation on Disk Chemistry
The chemistry within a protoplanetary disk is greatly affected by external radiation from the local stellar environment. Previous work has focused on extreme radiation fields, representative of the center of something like the Orion Nebula Cluster ...
Rachel E. Gross, L. Ilsedore Cleeves
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Semiempirical Potential in Kinetics Calculations on the HC3N + CN Reaction. [PDF]
Valença Ferreira de Aragão E+5 more
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On the character of the chief line of the Nebula in Orion [PDF]
K. D. Naegamvala
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Enabling the Industrial Internet of Things to Cloud Continuum in a Real City Environment. [PDF]
Cabrini FH+6 more
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On the Spectrum of the Great Nebula in Orion, and on the Motions of some Stars Towards or from the Earth* [PDF]
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Expanding bubbles in Orion A: [C <sub>II</sub>] observations of M42, M43, and NGC 1977. [PDF]
Pabst CHM+9 more
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Hidden Binaries in Star-forming Regions
A significant fraction of, and possibly all, stars form in binary or multiple systems. For solar-mass stars in the Galactic field, the distribution of orbital separations is log-normal over 7 orders of magnitude, from 10 ^−2 to 10 ^5 au.
Mary H. Rawcliffe+2 more
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The Trapezium in the great nebula of Orion. Great shower of falling stars [PDF]
W. F. Denning
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The SDSS-V Local Volume Mapper: Data Analysis Pipeline
We introduce the data analysis pipeline (DAP) for the Sloan Digital Sky Survey V Local Volume Mapper (LVM) project, referred to as the LVM-DAP. We outline our methods for recovering both stellar and emission-line components from optical integral field ...
Sebastián F. Sánchez+12 more
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Radial Velocities Within the Great Nebula of Orion [PDF]
Edwin B. Frost
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