Search Publications

Relativistic Lines and Reflection from the Inner Accretion Disks Around Neutron Stars
DOI: 10.1088/0004-637X/720/1/205 Bibcode: 2010ApJ...720..205C

Miller, Jon M.; Cackett, Edward M.; Wijnands, Rudy +6 more

A number of neutron star low-mass X-ray binaries (LMXBs) have recently been discovered to show broad, asymmetric Fe K emission lines in their X-ray spectra. These lines are generally thought to be the most prominent part of a reflection spectrum, originating in the inner part of the accretion disk where strong relativistic effects can broaden emis…

2010 The Astrophysical Journal
Suzaku XMM-Newton 173
Fermi Large Area Telescope View of the Core of the Radio Galaxy Centaurus A
DOI: 10.1088/0004-637X/719/2/1433 Bibcode: 2010ApJ...719.1433A

Ozaki, M.; Caraveo, P. A.; Frailis, M. +195 more

We present γ-ray observations with the Large Area Telescope (LAT) on board the Fermi Gamma-Ray Space Telescope of the nearby radio galaxy Centaurus A (Cen A). The previous EGRET detection is confirmed, and the localization is improved using data from the first 10 months of Fermi science operation. In previous work, we presented the detection of th…

2010 The Astrophysical Journal
Suzaku 167
Discovery of Ultra-fast Outflows in a Sample of Broad-line Radio Galaxies Observed with Suzaku
DOI: 10.1088/0004-637X/719/1/700 Bibcode: 2010ApJ...719..700T

Cappi, M.; Ballo, L.; Tombesi, F. +5 more

We present the results of a uniform and systematic search for blueshifted Fe K absorption lines in the X-ray spectra of five bright broad-line radio galaxies observed with Suzaku. We detect, for the first time in radio-loud active galactic nuclei (AGNs) at X-rays, several absorption lines at energies greater than 7 keV in three out of five sources…

2010 The Astrophysical Journal
Suzaku 162
Efficient Cosmic Ray Acceleration, Hydrodynamics, and Self-Consistent Thermal X-Ray Emission Applied to Supernova Remnant RX J1713.7-3946
DOI: 10.1088/0004-637X/712/1/287 Bibcode: 2010ApJ...712..287E

Raymond, John; Slane, Patrick; Ellison, Donald C. +1 more

We model the broadband emission from supernova remnant (SNR) RX J1713.7-3946 including, for the first time, a consistent calculation of thermal X-ray emission together with non-thermal emission in a nonlinear diffusive shock acceleration model. Our model tracks the evolution of the SNR including the plasma ionization state between the forward shoc…

2010 The Astrophysical Journal
Suzaku 161
Suzaku Observation of A1689: Anisotropic Temperature and Entropy Distributions Associated with the Large-scale Structure
DOI: 10.1088/0004-637X/714/1/423 Bibcode: 2010ApJ...714..423K

Fukazawa, Yasushi; Nakazawa, Kazuhiro; Ohashi, Takaya +7 more

We present results of new, deep Suzaku X-ray observations (160 ks) of the intracluster medium (ICM) in A1689 out to its virial radius, combined with complementary data sets of the projected galaxy distribution obtained from the SDSS catalog and the projected mass distribution from our recent comprehensive weak and strong lensing analysis of Subaru…

2010 The Astrophysical Journal
Suzaku XMM-Newton eHST 124
Expansion Velocity of Ejecta in Tycho's Supernova Remnant Measured by Doppler Broadened X-ray Line Emission
DOI: 10.1088/0004-637X/725/1/894 Bibcode: 2010ApJ...725..894H

Katsuda, Satoru; Kunieda, Hideyo; Makishima, Kazuo +10 more

We show that the expansion of ejecta in Tycho's supernova remnant (SNR) is consistent with a spherically symmetric shell, based on Suzaku measurements of the Doppler broadened X-ray emission lines. All of the strong Kα line emissions show broader widths at the center than at the rim, while the centroid energies are constant across the remnant (exc…

2010 The Astrophysical Journal
Suzaku 101
Galaxy Clusters at the Edge: Temperature, Entropy, and Gas Dynamics Near the Virial Radius
DOI: 10.1088/0004-637X/721/2/1105 Bibcode: 2010ApJ...721.1105B

O'Shea, Brian W.; Burns, Jack O.; Skillman, Samuel W.

Recently, Suzaku has produced temperature and entropy profiles, along with profiles of gas density, gas fraction, and mass, for multiple galaxy clusters out to approximately the virial radius. In this paper, we compare these novel X-ray observations with results from N-body + hydrodynamic adaptive mesh refinement cosmological simulations using the…

2010 The Astrophysical Journal
Suzaku 87
Dark Matter Search Using Chandra Observations of Willman 1 and a Spectral Feature Consistent with a Decay Line of a 5 keV Sterile Neutrino
DOI: 10.1088/0004-637X/714/1/652 Bibcode: 2010ApJ...714..652L

Loewenstein, Michael; Kusenko, Alexander

We report the results of a search for an emission line from radiatively decaying dark matter in the Chandra X-ray Observatory spectrum of the ultra-faint dwarf spheroidal galaxy Willman 1. 99% confidence line flux upper limits over the 0.4-7 keV Chandra bandpass are derived and mapped to an allowed region in the sterile neutrino mass-mixing angle …

2010 The Astrophysical Journal
Suzaku 79
Broadband Study with Suzaku of the Magnetar Class
DOI: 10.1088/2041-8205/722/2/L162 Bibcode: 2010ApJ...722L.162E

Hurley, K.; Rea, N.; Enoto, T. +3 more

Broadband (0.8-70 keV) spectra of the persistent X-ray emission from nine magnetars were obtained with Suzaku, including three objects in apparent outburst. The soft X-ray component was detected from all of them, with a typical blackbody temperature of kT ~ 0.5 keV, while the hard-tail component, dominating above ~10 keV, was detected at ~1 mCrab …

2010 The Astrophysical Journal
Suzaku 76
Quiescent X-ray Emission From Cen X-4: A Variable Thermal Component
DOI: 10.1088/0004-637X/720/2/1325 Bibcode: 2010ApJ...720.1325C

Miller, Jon M.; Cackett, Edward M.; Wijnands, Rudy +1 more

The nearby neutron star low-mass X-ray binary, Cen X-4, has been in a quiescent state since its last outburst in 1979. Typically, quiescent emission from these objects consists of thermal emission (presumably from the neutron star surface) with an additional hard power-law tail of unknown nature. Variability has been observed during quiescence in …

2010 The Astrophysical Journal
Suzaku XMM-Newton 72