Search Publications
A Search for Iron Emission Lines in the Chandra X-Ray Spectra of Neutron Star Low-Mass X-Ray Binaries
Wijnands, R.; Miller, J. M.; Homan, J. +6 more
While iron emission lines are well studied in black hole systems, both in X-ray binaries and active galactic nuclei, there has been less of a focus on these lines in neutron star low-mass X-ray binaries (LMXBs). However, recent observations with Suzaku and XMM-Newton have revealed broad, asymmetric iron line profiles in three neutron star LMXBs, c…
Albedo control of seasonal South Polar cap recession on Mars
Bibring, Jean-Pierre; Langevin, Yves; Schmitt, Bernard +4 more
Over the last few decades, General Circulation Models (GCM) have been used to simulate the current martian climate. The calibration of these GCMs with the current seasonal cycle is a crucial step in understanding the climate history of Mars. One of the main climatic signals currently used to validate GCMs is the annual atmospheric pressure cycle. …
Spitzer Observations of The H II Region NGC 2467: An Analysis of Triggered Star Formation
Bally, John; Hester, J. Jeff; Desch, Steven J. +2 more
We present new Spitzer Space Telescope observations of the region NGC 2467, and use these observations to determine how the environment of an H II region affects the process of star formation. Our observations comprise IRAC (3.6, 4.5, 5.8, and 8.0 µm) and MIPS (24 µm) maps of the region, covering approximately 400 arcmin2. T…
Characteristic Dependence of Umbral Dots on Their Magnetic Structure
Ichimoto, K.; Kitai, R.; Watanabe, H.
Umbral dots (UDs) were observed in a stable sunspot in NOAA 10944 by the Hinode Solar Optical Telescope on 2007 March 1. The observation program consisted of blue continuum images and spectropolarimetric profiles of Fe I 630 nm line. An automatic detection algorithm for UDs was applied to the 2 hr continuous blue continuum images, and using the ob…
Disentangling the Circumnuclear Environs of Centaurus A. I. High-Resolution Molecular Gas Imaging
Iono, D.; Espada, D.; Petitpas, G. +8 more
We present high-resolution images of the 12CO(2-1) emission in the central 1' (1 kpc) of NGC 5128 (Centaurus A), observed using the Submillimeter Array. We elucidate for the first time the distribution and kinematics of the molecular gas in this region with a resolution of 6farcs0 × 2farcs4 (100 pc × 40 pc). We spatially resolve the cir…
A Wide-Field Study of the z ~ 0.8 Cluster RX J0152.7-1357: The Role of Environment in the Formation of the Red Sequence
Franx, Marijn; Kelson, Daniel D.; Illingworth, Garth D. +4 more
We present the first results from the largest spectroscopic survey to date of an intermediate redshift galaxy cluster, the z = 0.834 cluster RX J0152.7-1357. We use the colors of galaxies, assembled from a D ~ 12 Mpc region centered on the cluster, to investigate the properties of the red sequence as a function of density and clustercentric radius…
Dissecting the Region of 3EG J1837-0423 and HESS J1841-055 with INTEGRAL
Masetti, N.; Bird, A. J.; Bassani, L. +3 more
3EG J1837-0423 and HESS J1841-055 are two unidentified and peculiar high-energy sources located in the same region of the sky, separated by ~1.4°. Specifically, 3EG J1837-0423 is a transient MeV object detected by EGRET only once during flaring activity that lasted a few days while HESS J1841-055 is a highly extended TeV source. We attempted to ma…
Quantitative estimates of the slab and 2-D power in solar wind turbulence using multispacecraft data
Horbury, T. S.; Osman, K. T.
A quantitative estimate of the field-aligned anisotropy of magnetohydrodynamic inertial range turbulence is obtained by comparing multispacecraft data with a fully three-dimensional turbulent magnetic field numerical model. The simulated turbulence is a superposition of slab fluctuations parallel to the mean field and 2-D fluctuations perpendicula…
Augmented Empirical Models of Plasmaspheric Density and Electric Field Using IMAGE and CLUSTER Data
Gallagher, Dennis L.; Tu, Jiannan; Moldwin, Mark B. +4 more
Empirical models for the plasma densities in the inner magnetosphere, including plasmasphere and polar magnetosphere, have been in the past derived from in situ measurements. Such empirical models, however, are still in their initial phase compared to magnetospheric magnetic field models. Recent studies using data from CRRES, Polar, and Image have…
The Dependence of Star Formation Activity on Stellar Mass Surface Density and Sersic Index in zCOSMOS Galaxies at 0.5 < z < 0.9 Compared with SDSS Galaxies at 0.04 < z < 0.08
Kneib, J. -P.; Maccagni, D.; Cimatti, A. +56 more
In order to try to understand the internal evolution of galaxies and relate this to the global evolution of the galaxy population, we present a comparative study of the dependence of star formation rates on the average surface mass densities (Σ M ) of galaxies at 0.5 < z < 0.9 and 0.04 < z < 0.08, using the zCOSMOS and Sloan…