10.4k citations
- United States Naval Research LaboratoryUS151 papers
- California Institute of TechnologyUS39 papers
- United States Naval ObservatoryUS39 papers
- Universidad de AlcaláES36 papers
- University of Maryland, College ParkUS36 papers
- Center for Astrophysics Harvard & SmithsonianUS35 papers
- Max Planck Institute for Extraterrestrial PhysicsDE35 papers
- Johns Hopkins UniversityUS33 papers
- University of ArizonaUS30 papers
- University of MichiganUS30 papers
- Princeton UniversityUS29 papers
- U.S. Naval Observatory Flagstaff StationUS29 papers
6 papers · 1 filter
Fundamental Parameters of 87 Stars from the Navy Precision Optical Interferometer
Ellyn K. Baines, J. Thomas Armstrong, Henrique R. Schmitt +5
We present the fundamental properties of 87 stars based on angular diameter measurements from the Navy Precision Optical Interferometer, 36 of which have not been measured previous…
Testing for Shock-Heated X-ray Gas Around Compact Steep Spectrum Radio Galaxies
C. P. O'Dea, D. M. Worrall, G. R. Tremblay +7
We present Chandra and XMM-Newton X-ray, VLA radio, and optical observations of three candidate Compact Steep Spectrum (CSS) radio galaxies. CSS sources are galactic scale and are…
Feedback and feeding in the context of galaxy evolution with SPICA: direct characterization of molecular outflows and inflows
E. González-Alfonso, L. Armus, F. J. Carrera +28
A far-infrared observatory such as the {\it SPace Infrared telescope for Cosmology and Astrophysics} ({\it SPICA}), with its unprecedented spectroscopic sensitivity, would unveil t…
Galaxy evolution studies with the SPace IR telescope for Cosmology and Astrophysics (SPICA): the power of IR spectroscopy
L. Spinoglio, A. Alonso-Herrero, L. Armus +65
IR spectroscopy in the range 12-230 micron with the SPace IR telescope for Cosmology and Astrophysics (SPICA) will reveal the physical processes that govern the formation and evolu…
SPICA and the Chemical Evolution of Galaxies: The Rise of Metals and Dust
J. A. Fernández-Ontiveros, L. Armus, M. Baes +33
The physical processes driving the chemical evolution of galaxies in the last cannot be understood without directly probing the dust-obscured phase of star-for…
Quasar Feedback in the Ultraluminous Infrared Galaxy F11119+3257: Connecting the Accretion Disk Wind with the Large-Scale Molecular Outflow
S. Veilleux, A. Bolatto, F. Tombesi +5
In Tombesi et al. (2015), we reported the first direct evidence for a quasar accretion disk wind driving a massive molecular outflow. The target was F11119+3257, an ultraluminous i…