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Spin-Down Measurement of PSR J1852+0040 in Kesteven 79: Central Compact Objects as Anti-Magnetars
DOI: 10.1088/0004-637X/709/1/436 Bibcode: 2010ApJ...709..436H

Gotthelf, E. V.; Halpern, J. P.

Using XMM-Newton and Chandra, we achieved phase-connected timing of the 105 ms X-ray pulsar PSR J1852+0040 that provides the first measurement of the spin-down rate of a member of the class of central compact objects (CCOs) in supernova remnants. We measure \dot{P} = (8.68 ± 0.09) × 10^{-18}, and find no evidence for timing noise or variations in …

2010 The Astrophysical Journal
XMM-Newton 171
Three-dimensional Solar WIND Modeling from the Sun to Earth by a SIP-CESE MHD Model with a Six-component Grid
DOI: 10.1088/0004-637X/723/1/300 Bibcode: 2010ApJ...723..300F

Wu, S. T.; Feng, Xueshang; Xiang, Changqing +3 more

The objective of this paper is to explore the application of a six-component overset grid to solar wind simulation with a three-dimensional (3D) Solar-InterPlanetary Conservation Element/Solution Element MHD model. The essential focus of our numerical model is devoted to dealing with: (1) the singularity and mesh convergence near the poles via the…

2010 The Astrophysical Journal
SOHO 168
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
Reconnection Outflows and Current Sheet Observed with Hinode/XRT in the 2008 April 9 "Cartwheel CME" Flare
DOI: 10.1088/0004-637X/722/1/329 Bibcode: 2010ApJ...722..329S

Reeves, Katharine K.; Longcope, Dana W.; Savage, Sabrina L. +2 more

Supra-arcade downflows (SADs) have been observed with Yohkoh/SXT (soft X-rays (SXR)), TRACE (extreme ultraviolet (EUV)), SOHO/LASCO (white light), SOHO/SUMER (EUV spectra), and Hinode/XRT (SXR). Characteristics such as low emissivity and trajectories, which slow as they reach the top of the arcade, are consistent with post-reconnection magnetic fl…

2010 The Astrophysical Journal
Hinode SOHO 166
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
A Massive Molecular Gas Reservoir in the z = 5.3 Submillimeter Galaxy AzTEC-3
DOI: 10.1088/2041-8205/720/2/L131 Bibcode: 2010ApJ...720L.131R

Schinnerer, Eva; Neri, Roberto; Scoville, Nicholas Z. +6 more

We report the detection of CO J = 2→1, 5→4, and 6→5 emission in the highest-redshift submillimeter galaxy (SMG) AzTEC-3 at z = 5.298, using the Expanded Very Large Array and the Plateau de Bure Interferometer. These observations ultimately confirm the redshift, making AzTEC-3 the most submillimeter-luminous galaxy in a massive z ~= 5.3 protocluste…

2010 The Astrophysical Journal
eHST 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
Imaging the Molecular Gas in a Submillimeter Galaxy at z = 4.05: Cold Mode Accretion or a Major Merger?
DOI: 10.1088/0004-637X/714/2/1407 Bibcode: 2010ApJ...714.1407C

Daddi, E.; Elbaz, D.; Stern, D. +11 more

We present a high-resolution (down to 0farcs18), multi-transition imaging study of the molecular gas in the z = 4.05 submillimeter galaxy GN20. GN20 is one of the most luminous starburst galaxy known at z>4, and is a member of a rich proto-cluster of galaxies at z = 4.05 in GOODS-North. We have observed the CO 1-0 and 2-1 emission with the Very…

2010 The Astrophysical Journal
eHST 160
A Short Gamma-ray Burst "No-host" Problem? Investigating Large Progenitor Offsets for Short GRBs with Optical Afterglows
DOI: 10.1088/0004-637X/722/2/1946 Bibcode: 2010ApJ...722.1946B

Berger, E.

We investigate the afterglow properties and large-scale environments of several short-duration gamma-ray bursts (GRBs) with subarcsecond optical afterglow positions but no bright coincident host galaxies. The purpose of this joint study is to robustly assess the possibility of significant offsets, a hallmark of the compact object binary merger mod…

2010 The Astrophysical Journal
eHST 158
The ACS Fornax Cluster Survey. VIII. The Luminosity Function of Globular Clusters in Virgo and Fornax Early-type Galaxies and Its Use as a Distance Indicator
DOI: 10.1088/0004-637X/717/2/603 Bibcode: 2010ApJ...717..603V

Jordán, Andrés; Infante, Leopoldo; Tonry, John L. +8 more

We use a highly homogeneous set of data from 132 early-type galaxies in the Virgo and Fornax clusters in order to study the properties of the globular cluster luminosity function (GCLF). The globular cluster system of each galaxy was studied using a maximum likelihood approach to model the intrinsic GCLF after accounting for contamination and comp…

2010 The Astrophysical Journal
eHST 157