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Cyclotron Resonance Energies at a Low X-Ray Luminosity: A0535+262 Observed with Suzaku
DOI: 10.1086/508018 Bibcode: 2006ApJ...648L.139T

Mukai, K.; Yonetoku, D.; Mihara, T. +28 more

The binary X-ray pulsar A0535+262 was observed with the Suzaku X-ray observatory on 2005 September 14 for a net exposure of 22 ks. The source was in the declining phase of a minor outburst, exhibiting 3-50 keV luminosity of ~3.7×1035 ergs s-1 at an assumed distance of 2 kpc. In spite of the very low source intensity (about 30…

2006 The Astrophysical Journal
Suzaku 53
On the Feedback from Super Stellar Clusters. I. The Structure of Giant H II Regions and H II Galaxies
DOI: 10.1086/502644 Bibcode: 2006ApJ...643..186T

Tenorio-Tagle, Guillermo; Muñoz-Tuñón, Casiana; Pérez, Enrique +2 more

We review the structural properties of giant extragalactic H II regions and H II galaxies based on two-dimensional hydrodynamic calculations and propose an evolutionary sequence that accounts for their observed detailed structure. The model assumes a massive and young stellar cluster surrounded by a large collection of clouds. These are thus expos…

2006 The Astrophysical Journal
eHST 53
Statistical Analysis of Reconnection Inflows in Solar Flares Observed with SOHO EIT
DOI: 10.1086/498492 Bibcode: 2006ApJ...637.1122N

Shibata, Kazunari; Narukage, Noriyuki

We report observations of reconnection inflows in extreme ultraviolet (EUV) Fe XII λ195 images with the Extreme Ultraviolet Imaging Telescope (EIT) on board the Solar and Heliospheric Observatory (SOHO). Yokoyama and colleagues reported the first example observed on 1999 March 18. We survey the EIT data from 1996 to 2000 and find six new inflow ev…

2006 The Astrophysical Journal
SOHO 53
Binary and Multiple O-Type Stars in the Cassiopeia OB6 Association
DOI: 10.1086/499771 Bibcode: 2006ApJ...639.1069H

Gies, Douglas R.; Bagnuolo, William G., Jr.; McSwain, M. Virginia +3 more

We present the results of time-resolved spectroscopy of 13 O-type stars in the Cas OB6 stellar association. We conducted a survey for radial velocity variability in search of binary systems, which are expected to be plentiful in young OB associations. Here we report the discovery of two new single-lined binaries, and we present new orbital element…

2006 The Astrophysical Journal
IUE 53
Type II Quasars from the Sloan Digital Sky Survey. IV. Chandra and XMM-Newton Observations Reveal Heavily Absorbed Sources
DOI: 10.1086/498233 Bibcode: 2006ApJ...637..147P

Strauss, Michael A.; Schneider, Donald P.; Heckman, Timothy M. +4 more

We are carrying out sensitive X-ray observations with Chandra and XMM-Newton of type II quasars selected from the Sloan Digital Sky Survey based on their optical emission line properties. In this paper we present the first results of our program. We present observations of four objects at redshifts 0.4<z<0.8, and an analysis of the archival …

2006 The Astrophysical Journal
XMM-Newton 52
Extinction Columns and Intrinsic X-Ray Spectra of the Anomalous X-Ray Pulsars
DOI: 10.1086/507174 Bibcode: 2006ApJ...650.1082D

Durant, Martin; van Kerkwijk, Marten H.

The X-ray spectra of anomalous X-ray pulsars have long been fit by smooth, empirical models such as the sum of a blackbody plus a power law. These reproduce the ~0.5-10 keV range well, but fail at lower and higher energies, grossly overpredicting the optical and underpredicting the hard X-ray emission. A poorly constrained source of uncertainty in…

2006 The Astrophysical Journal
XMM-Newton 52
The Sunyaev-Zel'dovich Effect in a Sample of 31 Clusters: A Comparison between the X-Ray Predicted and WMAP Observed Cosmic Microwave Background Temperature Decrement
DOI: 10.1086/505627 Bibcode: 2006ApJ...648..176L

Zhang, Shuang-Nan; Lieu, Richard; Mittaz, Jonathan P. D.

The WMAP Q-, V-, and W-band radial profiles of temperature deviation of the cosmic microwave background (CMB) were constructed for a sample of 31 randomly selected nearby clusters of galaxies in directions of Galactic latitude b>30deg. The profiles were compared in detail with the expected CMB Sunyaev-Zel'dovich effect (SZE) caused b…

2006 The Astrophysical Journal
XMM-Newton 51
Impact of Major Coronal Mass Ejections on Geospace during 2005 September 7-13
DOI: 10.1086/504676 Bibcode: 2006ApJ...646..625W

Wang, Yuming; Shen, Chenglong; Wang, S. +3 more

We have analyzed five major CMEs originating from NOAA active region (AR) 808 during the period of 2005 September 7-13, when the AR 808 rotated from the east limb to near solar meridian. Several factors that affect the probability of the CMEs' encounter with the Earth are demonstrated. The solar and interplanetary observations suggest that the sec…

2006 The Astrophysical Journal
SOHO 51
The Polar Regions of Cassiopeia A: The Aftermath of a Gamma-Ray Burst?
DOI: 10.1086/503553 Bibcode: 2006ApJ...644..260L

Hwang, Una; Laming, J. Martin; Radics, Balint +2 more

Are the polar regions of Cas A the aftermath of a gamma-ray burst? Probably not, but it is interesting nevertheless to investigate just how close Cas A might have come to generating such an event. Focusing on the northeast jet filaments, we analyze the polar regions of the recently acquired very deep 1 Ms Chandra X-ray observation. We infer that t…

2006 The Astrophysical Journal
eHST 51
p-Mode Propagation through the Transition Region into the Solar Corona. I. Observations
DOI: 10.1086/501450 Bibcode: 2006ApJ...643..540M

Marsh, M. S.; Walsh, R. W.

Oscillations have long been observed in the sunspot umbral chromosphere and transition region, connected to global p-mode oscillations. These p-modes are thought to undergo mode conversion to slow magnetoacoustic waves in regions of strong magnetic field. More recently, propagating oscillations have also been observed in solar coronal loops. Using…

2006 The Astrophysical Journal
SOHO 50