Results 101 to 110 of about 419,985 (168)

Tomography of ultrarelativistic nuclei with polarized photon-gluon collisions. [PDF]

Sci Adv, 2023
STAR Collaboration.
europepmc   +1 more source

["Starlight" Zebras Music Video]

, 1984
A video of multiple cuts of the Zebras performing "Starlight.
University of North Texas. Center for Media Production.
core  

Dust and Starlight Maps for Galaxies in the KINGFISH Sample

, 2019
Dust and starlight have been modeled for the KINGFISH project galaxies. For each pixel in each galaxy, we estimate: (1) dust surface density; (2) q_PAH, the dust mass fraction in PAHs; (3) distribution of starlight intensities heating the dust; (4 ...
Boquien, M., Kennicutt, R.C., Smith, J.-D.T., Koda, J., Hinz, J., Roussel, H., Bolatto, A.D., Galametz, M., Armus, L., Gordon, K.D., Walter, F., Wolfire, M.G., Miller, A., Relano, M., Schinnerer, E., De Looze, I., Leroy, A.K., Montiel, E., Murphy, E.J., Sandstrom, K., Crocker, A., Aniano, G., Sauvage, M., Skibba, R., Hunt, L.K., Johnson, B.D., Engelbracht, C.W., Helou, G., Donovan Meyer, J., Rix, H.-W., Calzetti, D., Draine, B.T., Dale, D.A.   +32 more
core   +1 more source

Linear Polarization of Synchrotron Radiation from Very-small-pitch-angle Electrons

The Astrophysical Journal
For synchrotron radiation with pitch angle α  ≪ 1/ γ where γ is the electron Lorentz factor, referred to as very-small-pitch-angle synchrotron radiation, the polarization properties differ significantly from those of conventional synchrotron radiation ...
Meng Nie, Jirong Mao
doaj   +1 more source

Demo 24-04 Microwave Polarization

, 2001
This demonstration illustrates one mechanism for the polarization of electromagnetic waves, using the apparatus as shown in Figure 1. The result is counterintuitive in that the waves that pass through the polarizer are polarized perpendicular to the ...

core  

Variable Linear Polarization across Optical Emission Lines of the Wolf–Rayet Star EZ Canis Majoris and Its Relation to Corotating Interaction Regions

The Astrophysical Journal
Structure can be found on all scales in the winds of hot, luminous stars, including Wolf–Rayet (W-R) stars. Large-scale, spiral-shaped corotating interaction regions (CIRs) are thought to be present, causing quasi-periodic variability.
L. Fabiani, N. St-Louis, A. F. J. Moffat, A-N. Chené, R. Ignace   +4 more
doaj   +1 more source

Starlight

, 1939
Black and white photograph of bay mare Starlight during early season workouts at Narragansett Park, Gorham Fair Grounds in 1939.https://digitalcommons.library.umaine.edu/kendall_images/3512/thumbnail ...
Kendall, Guy
core  

Spectropolarimetric Evolution Reveals Dual-axis Ejecta in the Atypical Magnetar-powered SN 2012au

The Astrophysical Journal
We present six epochs of optical spectropolarimetric observations of the unique and slow-evolving Type Ib supernova (SN) 2012au, between 0 and 295 day post- R -band maximum.
Sabrina DeSoto, Jennifer L. Hoffman, G. Grant Williams, Christopher Bilinski, Douglas C. Leonard, Peter A. Milne, Christopher Pickens, Manisha Shrestha, Nathan Smith, Paul S. Smith   +9 more
doaj   +1 more source

A 3D Attitude Estimation Method Based on Attitude Angular Partial Feedback for Polarization-Based Integrated Navigation System. [PDF]

Sensors (Basel), 2022
Hu P, Huang P, Qiu Z, Yang J, Liu X.
europepmc   +1 more source

Setting Boundaries for Statistical Mechanics. [PDF]

Molecules, 2022
Eisenberg B.
europepmc   +1 more source