Search Publications

The Jet Heated X-Ray Filament in the Centaurus A Northern Middle Radio Lobe
DOI: 10.1088/0004-637X/698/2/2036 Bibcode: 2009ApJ...698.2036K

Hardcastle, M. J.; Croston, J. H.; Birkinshaw, M. +6 more

We present results from a 40 ks XMM-Newton observation of the X-ray filament coincident with the southeast edge of the Centaurus A Northern Middle Radio Lobe (NML). We find that the X-ray filament consists of five spatially resolved X-ray knots embedded in a continuous diffuse bridge. The spectrum of each knot is well fitted by a thermal model wit…

2009 The Astrophysical Journal
XMM-Newton 46
Suzaku View of the Swift/BAT Active Galactic Nuclei. I. Spectral Analysis of Six Active Galactic Nuclei and Evidence for Two Types of Obscured Population
DOI: 10.1088/0004-637X/696/2/1657 Bibcode: 2009ApJ...696.1657E

Ueda, Yoshihiro; Terashima, Yuichi; Mushotzky, Richard +2 more

We present a systematic spectral analysis with Suzaku of six active galactic nuclei (AGNs) detected in the Swift/BAT hard X-ray (15-200 keV) survey: Swift J0138.6-4001, J0255.2-0011, J0350.1-5019, J0505.7-2348, J0601.9-8636, and J1628.1-5145. This is considered to be a representative sample of new AGNs without X-ray spectral information before the…

2009 The Astrophysical Journal
Suzaku 46
Tools for Dissecting Supernova Remnants Observed with Chandra: Methods and Application to the Galactic Remnant W49B
DOI: 10.1088/0004-637X/691/1/875 Bibcode: 2009ApJ...691..875L

Ramirez-Ruiz, E.; Jeltema, T. E.; Lopez, L. A. +1 more

We introduce methods to quantify the X-ray morphologies of supernova remnants (SNRs) observed with the Chandra X-ray Telescope. These include a power-ratio technique to measure morphological asymmetries, correlation-length analysis to probe chemical segregation and distribution, and wavelet-transform analysis to quantify the X-ray substructure. We…

2009 The Astrophysical Journal
XMM-Newton 45
Temperature Tomography of a Coronal Sigmoid Supporting the Gradual Formation of a Flux Rope
DOI: 10.1088/0004-637X/698/1/L27 Bibcode: 2009ApJ...698L..27T

Young, Peter R.; Tripathi, Durgesh; Kliem, Bernhard +2 more

Multiwavelength observations of a sigmoidal (S-shaped) solar coronal source by the EUV Imaging Spectrometer and the X-Ray Telescope aboard the Hinode spacecraft and by the EUV Imager aboard STEREO are reported. The data reveal the coexistence of a pair of J-shaped hot arcs at temperatures T>2 MK with an S-shaped structure at somewhat lower temp…

2009 The Astrophysical Journal
Hinode 45
The Dusty Nuclear Torus in NGC 4151: Constraints from Gemini Near-Infrared Integral Field Spectrograph Observations
DOI: 10.1088/0004-637X/698/2/1767 Bibcode: 2009ApJ...698.1767R

Storchi-Bergmann, Thaisa; Riffel, Rogemar A.; McGregor, Peter J.

We have used a near-infrared (near-IR) nuclear spectrum (covering the Z, J, H, and K bands) of the nucleus of NGC 4151 obtained with the Gemini Near-Infrared Integral Field Spectrograph (NIFS) and adaptive optics, to isolate and constrain the properties of a near-IR unresolved nuclear source whose spectral signature is clearly present in our data.…

2009 The Astrophysical Journal
eHST 45
Hydrostatic Gas Constraints on Supermassive Black Hole Masses: Implications for Hydrostatic Equilibrium and Dynamical Modeling in a Sample of Early-type Galaxies
DOI: 10.1088/0004-637X/703/2/1257 Bibcode: 2009ApJ...703.1257H

Gebhardt, Karl; Humphrey, Philip J.; Buote, David A. +2 more

We present new mass measurements for the supermassive black holes (SMBHs) in the centers of three early-type galaxies. The gas pressure in the surrounding, hot interstellar medium (ISM) is measured through spatially resolved spectroscopy with the Chandra X-ray Observatory, allowing the SMBH mass (M BH) to be inferred directly under the …

2009 The Astrophysical Journal
eHST 45
X-ray Spectroscopy of the Core of the Perseus Cluster with Suzaku: Elemental Abundances in the Intracluster Medium
DOI: 10.1088/0004-637X/705/1/L62 Bibcode: 2009ApJ...705L..62T

Fabian, A. C.; Mitsuda, K.; Sanders, J. S. +7 more

The results from Suzaku observations of the central region of the Perseus cluster are presented. Deep exposures with the X-ray Imaging Spectrometer provide high-quality X-ray spectra from the intracluster medium. X-ray lines from helium-like Cr and Mn have been detected significantly for the first time in clusters. In addition, elemental abundance…

2009 The Astrophysical Journal
Suzaku 45
A Statistical Study of Hard X-Ray Footpoint Motions in Large Solar Flares
DOI: 10.1088/0004-637X/693/1/132 Bibcode: 2009ApJ...693..132Y

Krucker, Säm; Ip, W. H.; Lin, R. P. +2 more

A statistical analysis of the temporal evolution of hard X-ray (HXR) footpoint motions in 27 M- and X-class solar flares observed by the Reuven Ramaty High Energy Solar Spectroscopic Imager is presented. Extreme UV images from TRACE and SOHO/EIT, Hα images, and magnetograms from SOHO/MDI are used to put the HXR footpoint motions in context of flar…

2009 The Astrophysical Journal
SOHO 44
Long-Term Stability of Nonthermal X-Ray Modulation in the Gamma-Ray Binary LS 5039
DOI: 10.1088/0004-637X/697/1/L1 Bibcode: 2009ApJ...697L...1K

Takahashi, Tadayuki; Uchiyama, Yasunobu; Tanaka, Takaaki +1 more

We report on long-term stability of X-ray modulation apparently synchronized with an orbital period of 3.9 days in the γ-ray binary LS 5039. Recent observations with the Suzaku satellite in the year 2007, which continuously covered more than one orbital period, have provided us with detailed characterization of X-ray flux and spectral shape as a f…

2009 The Astrophysical Journal
Suzaku XMM-Newton 44
Color Distributions, Number, and Mass Densities of Massive Galaxies at 1.5 < z < 3: Comparing Observations with Merger Simulations
DOI: 10.1088/0004-637X/700/1/799 Bibcode: 2009ApJ...700..799W

van Dokkum, Pieter G.; Franx, Marijn; Labbé, Ivo +9 more

We present a comparison between the observed color distribution, number, and mass density of massive galaxies at 1.5 < z < 3 and a model by Hopkins et al. that relates the quasar and galaxy population on the basis of gas-rich mergers. In order to test the hypothesis that quiescent red galaxies are formed after a gas-rich merger involving qua…

2009 The Astrophysical Journal
eHST 44