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X-ray Emission from Nitrogen-Type Wolf-Rayet Stars
DOI: 10.1088/0004-6256/139/3/825 Bibcode: 2010AJ....139..825S

Skinner, Stephen L.; Zhekov, Svetozar A.; Güdel, Manuel +2 more

We summarize new X-ray detections of four nitrogen-type Wolf-Rayet (WR) stars obtained in a limited survey aimed at establishing the X-ray properties of WN stars across their full range of spectral subtypes. None of the detected stars is so far known to be a close binary. We report Chandra detections of WR 2 (WN2), WR 18 (WN4), and WR 134 (WN6), a…

2010 The Astronomical Journal
XMM-Newton 61
Morphologies of Radio-, X-ray-, and Mid-infrared-selected Active Galactic Nuclei
DOI: 10.1088/0004-6256/140/2/533 Bibcode: 2010AJ....140..533G

Griffith, Roger L.; Stern, Daniel

We investigate the optical morphologies of candidate active galaxies identified at radio, X-ray, and mid-infrared wavelengths. We use the Advanced Camera for Surveys General Catalog (ACS-GC) to identify 372, 1360, and 1238 active galactic nucleus (AGN) host galaxies from Very Large Array, XMM-Newton, and Spitzer Space Telescope observations of the…

2010 The Astronomical Journal
XMM-Newton eHST 46
Hard X-ray Emission Associated with White Dwarfs. III.
DOI: 10.1088/0004-6256/140/5/1433 Bibcode: 2010AJ....140.1433B

Chu, You-Hua; Bilíková, Jana; Gruendl, Robert A. +1 more

Hard X-ray emission associated with white dwarfs (WDs) can be used to diagnose the presence of late-type binary companions, mass accretion from companions, or physical processes with unknown origins. Since our previous systematic searches for hard X-ray emission associated with WDs, the Galactic WD catalog has been augmented by >10,000 new WDs …

2010 The Astronomical Journal
XMM-Newton 27
Simultaneous X-ray and Ultraviolet Observations of the SW Sextantis Star DW Ursae Majoris
DOI: 10.1088/0004-6256/140/5/1313 Bibcode: 2010AJ....140.1313H

Dhillon, V. S.; Szkody, Paula; Hoard, D. W. +6 more

We present the first pointed X-ray observation of DW Ursae Majoris, a novalike cataclysmic variable (CV) and one of the archetype members of the SW Sextantis class, obtained with the XMM-Newton satellite. These data provide the first detailed look at an SW Sex star in the X-ray regime (with previous X-ray knowledge of the SW Sex stars limited prim…

2010 The Astronomical Journal
XMM-Newton 16
Spitzer Observations of A1763. II. Constraining the Nature of Activity in the Cluster-feeding Filament with VLA and XMM-Newton Data
DOI: 10.1088/0004-6256/140/6/1891 Bibcode: 2010AJ....140.1891E

Fadda, Dario; Frayer, David T.; Durret, Florence +2 more

The A1763 superstructure at z = 0.23 contains the first galaxy filament to be directly detected using mid-infrared observations. Our previous work has shown that the frequency of starbursting galaxies, as characterized by 24 µm emission is much higher within the filament than at either the center of the rich galaxy cluster, or the field surr…

2010 The Astronomical Journal
XMM-Newton 10
XMM-Newton Observations of the Enigmatic Long Period Eclipsing Binary Epsilon Aurigæ: Constraining the Physical Models
DOI: 10.1088/0004-6256/140/2/595 Bibcode: 2010AJ....140..595W

Wolk, Scott J.; Guinan, Edward; Pillitteri, Ignazio +1 more

We report on an XMM-Newton observation of the unusual, long period (F0 supergiant + cool disk companion) eclipsing binary star epsilon Aurigæ observed in X-rays prior to the onset of the 2009-2011 eclipse phase. While it appears certain that a disk-like body is obscuring the star, it remains unclear what kind of object is at the center of the disk…

2010 The Astronomical Journal
XMM-Newton 6
Multiwavelength Observations of the Runaway Binary HD 15137
DOI: 10.1088/0004-6256/139/3/857 Bibcode: 2010AJ....139..857M

Gies, Douglas R.; Roettenbacher, Rachael M.; De Becker, Michaël +6 more

HD 15137 is an intriguing runaway O-type binary system that offers a rare opportunity to explore the mechanism by which it was ejected from the open cluster of its birth. Here, we present recent blue optical spectra of HD 15137 and derive a new orbital solution for the spectroscopic binary and physical parameters of the O star primary. We also pre…

2010 The Astronomical Journal
XMM-Newton 6
XMM-Newton Observations of the Radio-Loud Broad Absorption Line Quasar FBQS J131213.5+231958
DOI: 10.1088/0004-6256/140/6/1960 Bibcode: 2010AJ....140.1960M

Mathur, Smita; Dai, Xinyu

We present XMM-Newton observations of the broad absorption line (BAL) quasar FBQS J131213.5+231958. The X-ray spectrum of the source can be well described by an absorbed power-law model in which the absorber is either ionized or only partially covers the continuum source. This can explain the apparent lack of absorption observed in the Chandra spe…

2010 The Astronomical Journal
XMM-Newton 0