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High-resolution X-Ray Spectroscopy Reveals the Special Nature of Wolf-Rayet Star Winds
DOI: 10.1088/2041-8205/747/2/L25 Bibcode: 2012ApJ...747L..25O

Hamann, W. -R.; Oskinova, L. M.; Ignace, R. +3 more

We present the first high-resolution X-ray spectrum of a putatively single Wolf-Rayet (WR) star. 400 ks observations of WR 6 by the XMM-Newton telescope resulted in a superb quality high-resolution X-ray spectrum. Spectral analysis reveals that the X-rays originate far out in the stellar wind, more than 30 stellar radii from the photosphere, and t…

2012 The Astrophysical Journal
XMM-Newton 31
The Nature of the Bright ULX X-2 in NGC 3921: A Chandra Position and HST Candidate Counterpart
DOI: 10.1088/0004-637X/758/1/28 Bibcode: 2012ApJ...758...28J

Fabian, A. C.; Miniutti, G.; Miller-Jones, J. C. A. +6 more

We report on Chandra observations of the bright ultraluminous X-ray (ULX) source in NGC 3921. Previous XMM-Newton observations reported in the literature show the presence of a bright ULX at a 0.5-10 keV luminosity of 2 × 1040 erg s-1. Our Chandra observation finds the source at a lower luminosity of ≈8 × 1039 erg …

2012 The Astrophysical Journal
XMM-Newton eHST 31
Determination of the Heliospheric Radial Magnetic Field from the Standoff Distance of a CME-driven Shock Observed by the STEREO Spacecraft
DOI: 10.1088/0004-637X/758/2/118 Bibcode: 2012ApJ...758..118P

Gopalswamy, Nat; Yashiro, Seiji; Kwon, Ryun-Young +2 more

We report on the determination of radial magnetic field strength in the heliocentric distance range from 6 to 120 solar radii (R ) using data from Coronagraph 2 (COR2) and Heliospheric Imager I (HI1) instruments on board the Solar Terrestrial Relations Observatory spacecraft following the standoff-distance method of Gopalswamy & Ya…

2012 The Astrophysical Journal
SOHO 31
Discovery of a Kiloparsec-scale X-Ray/Radio Jet in the z = 4.72 Quasar GB 1428+4217
DOI: 10.1088/2041-8205/756/1/L20 Bibcode: 2012ApJ...756L..20C

Cheung, C. C.; Stawarz, Ł.; Siemiginowska, A. +4 more

We report the discovery of a one-sided 3farcs6 (24 kpc, projected) long jet in the high-redshift, z = 4.72, quasar GB 1428+4217 in new Chandra X-ray and Very Large Array (VLA) radio observations. This is the highest redshift kiloparsec-scale X-ray/radio jet known. Analysis of archival very long baseline interferometry 2.3 and 8.6 GHz data reveal a…

2012 The Astrophysical Journal
eHST 31
A Search for an Intermediate-mass Black Hole in the Core of the Globular Cluster NGC 6266
DOI: 10.1088/0004-637X/745/2/175 Bibcode: 2012ApJ...745..175M

Harrison, Thomas E.; Baumgardt, Holger; McNamara, Bernard J. +1 more

It has long been thought that intermediate-mass black holes (IMBHs) might be located in the cores of globular clusters. However, studies attempting to confirm this possibility have been inconclusive. To refine the search for these objects, Baumgardt et al. completed a series of N-body simulations to determine the observational properties that a ho…

2012 The Astrophysical Journal
eHST 31
Elemental Abundances in the Possible Type Ia Supernova Remnant G344.7-0.1
DOI: 10.1088/0004-637X/749/2/137 Bibcode: 2012ApJ...749..137Y

Yamaguchi, H.; Tanaka, M.; Maeda, K. +5 more

Recent studies on the Galactic supernova remnant (SNR) G344.7-0.1 have commonly claimed its origin to be a core-collapse supernova (SN) explosion, based on its highly asymmetric morphology and/or proximity to a star-forming region. In this paper, however, we present an X-ray spectroscopic study of this SNR using Suzaku, which is supportive of a Ty…

2012 The Astrophysical Journal
Suzaku 31
Deep Chandra Monitoring Observations of NGC 4649. II. Wide-field Hubble Space Telescope Imaging of the Globular Clusters
DOI: 10.1088/0004-637X/760/1/87 Bibcode: 2012ApJ...760...87S

Brodie, Jean P.; Zezas, Andreas; Strader, Jay +7 more

We present g and z photometry and size estimates for globular clusters (GCs) in the massive Virgo elliptical NGC 4649 (M60) using a five-pointing Hubble Space Telescope/Advanced Camera for Surveys mosaic. The metal-poor GCs show a monotonic negative metallicity gradient of -0.43 ± 0.10 dex per dex in radius over the full radial range of the data, …

2012 The Astrophysical Journal
eHST 31
Deep Hubble Space Telescope Imaging in NGC 6397: Stellar Dynamics
DOI: 10.1088/0004-637X/761/1/51 Bibcode: 2012ApJ...761...51H

Anderson, J.; Rich, R. M.; Dotter, A. +9 more

Multi-epoch observations with the Advanced Camera for Surveys on the Hubble Space Telescope provide a unique and comprehensive probe of stellar dynamics within NGC 6397. We are able to confront analytic models of the globular cluster with the observed stellar proper motions. The measured proper motions probe well along the main sequence from 0.8 t…

2012 The Astrophysical Journal
eHST 31
Hubble Space Telescope Narrowband Search for Extended Lyα Emission around Two z > 6 Quasars
DOI: 10.1088/0004-637X/756/2/150 Bibcode: 2012ApJ...756..150D

Hennawi, Joseph F.; Strauss, Michael A.; Rix, Hans-Walter +8 more

We search for extended Lyα emission around two z > 6 quasars, SDSS J1030+0524 (z = 6.309) and SDSS J1148+5251 (z = 6.419) using Wide Field Camera 3 narrowband filters on board the Hubble Space Telescope. For each quasar, we collected two deep, narrowband images, one sampling the Lyα line+continuum at the quasar redshifts and one of the continuu…

2012 The Astrophysical Journal
eHST 31
Spatially Dependent Heating and Ionization in an ICME Observed by Both ACE and Ulysses
DOI: 10.1088/0004-637X/760/2/105 Bibcode: 2012ApJ...760..105L

Laming, J. Martin; von Steiger, Rudolf; Rakowski, Cara E. +1 more

The 2005 January 21 interplanetary coronal mass ejection (ICME) observed by multiple spacecraft at L1 was also observed from January 21-February 4 at Ulysses (5.3 AU). Previous studies of this ICME have found evidence suggesting that the flanks of a magnetic cloud like structure associated with this ICME were observed at L1 while a more central cu…

2012 The Astrophysical Journal
Ulysses 30