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- Max Planck Institute for Gravitational PhysicsDE9 papers
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5 papers · 1 filter
Determination of the Coronal Magnetic Field by Hot Loop Oscillations
Tongjiang Wang, Davina E. Innes, Jiong Qiu
We apply a new method to determine the magnetic field in coronal loops using observations of coronal loop oscillations. We analyze seven Doppler shift oscillation events detected b…
A Solution to the Galactic Foreground Problem for LISA
Jeff Crowder, Neil Cornish
Low frequency gravitational wave detectors, such as the Laser Interferometer Space Antenna (LISA), will have to contend with large foregrounds produced by millions of compact galac…
Sloan/Johnson-Cousins/2MASS Color Transformations for Cool-Stars
James R. A. Davenport, Andrew A. West, Caleb K. Matthiesen +2
We present multi-color transformations and photometric parallaxes for a sample of 40 low mass dwarfs selected from the Sloan Digital Sky Survey (SDSS) and the General Catalog of Tr…
Senescence Can Explain Microbial Persistence
I. Klapper, P. Gilbert, B. P. Ayati +2
It has been known for many years that small fractions of persister cells resist killing in many bacterial colony-antimicrobial confrontations. These persisters are not believed to…
Production of high-energy μneutrinos from young neutron stars
G. F. Burgio, B. Link
Young, rapidly rotating neutron stars could accelerate protons to energies of PeV close to the stellar surface, which scatter with x-rays from the stellar surface through…