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- University of Maryland, College ParkUS243 papers
- Goddard Space Flight CenterUS141 papers
- Deleted Institution94 papers
- California Institute of TechnologyUS79 papers
- Centre National de la Recherche ScientifiqueFR48 papers
- University of California, BerkeleyUS46 papers
- Max Planck Institute for Extraterrestrial PhysicsDE42 papers
- Jet Propulsion LaboratoryUS39 papers
- Center for Astrophysics Harvard & SmithsonianUS36 papers
- University of CambridgeGB35 papers
- National Radio Astronomy ObservatoryUS31 papers
- University of SouthamptonGB31 papers
20 papers · 1 filter
The Radio Spectral Energy Distribution and Star Formation Rate Calibration in Galaxies
F. S. Tabatabaei, E. Schinnerer, M. Krause +17
We study the spectral energy distribution (SED) of the radio continuum emission from the KINGFISH sample of nearby galaxies to understand the energetics and origin of this emission…
iPTF Discovery of the Rapid "Turn On" of a Luminous Quasar
S. Gezari, T. Hung, S. B. Cenko +13
We present a radio-quiet quasar at z=0.237 discovered "turning on" by the intermediate Palomar Transient Factory (iPTF). The transient, iPTF 16bco, was detected by iPTF in the nucl…
Molecular outflows in local ULIRGs: energetics from multi-transition OH analysis
E. González-Alfonso, J. Fischer, H. W. W. Spoon +11
We report on the energetics of molecular outflows in 14 local Ultraluminous Infrared Galaxies (ULIRGs) that show unambiguous outflow signatures (P-Cygni profiles or high-velocity a…
Gravitational waves from f-modes excited by the inspiral of highly eccentric neutron star binaries
Cecilia Chirenti, Roman Gold, M. Coleman Miller
As gravitational wave instrumentation becomes more sensitive, it is interesting to speculate about subtle effects that could be analyzed using upcoming generations of detectors. On…
Millimeter-Wave Line Ratios and Sub-beam Volume Density Distributions
Adam K. Leroy, Antonio Usero, Andreas Schruba +11
We explore the use of mm-wave emission line ratios to trace molecular gas density when observations integrate over a wide range of volume densities within a single telescope beam.…
The Highest-Energy Cosmic Rays Cannot be Dominantly Protons from Steady Sources
Ke Fang, Kumiko Kotera
The bulk of observed ultrahigh energy cosmic rays could be light or heavier elements, and originate from an either steady or transient population of sources. This leaves us with fo…