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The X-Ray Eclipse Geometry of the Super-soft X-Ray Source CAL 87
DOI: 10.1088/0004-637X/792/1/20 Bibcode: 2014ApJ...792...20R

Lopes de Oliveira, R.; Ribeiro, T.; Borges, B. W.

We explore XMM-Newton observations of the eclipsing super-soft X-ray source CAL 87 in order to map the accretion structures of the system. Indirect imaging techniques were applied in X-ray light curves to provide eclipse maps. The surface brightness distribution exhibits an extended and symmetric emission, and a feature is revealed from the hardes…

2014 The Astrophysical Journal
XMM-Newton 8
Comparison of Galaxy Clusters Selected by Weak-lensing, Optical Spectroscopy, and X-Rays in the Deep Lens Survey F2 Field
DOI: 10.1088/0004-637X/786/2/125 Bibcode: 2014ApJ...786..125S

Jones, Christine; Geller, Margaret J.; Kurtz, Michael J. +6 more

We compare galaxy clusters selected in Chandra and XMM-Newton X-ray observations of the 4 deg2 Deep Lens Survey (DLS) F2 field to the cluster samples previously selected in the same field from a sensitive weak-lensing shear map derived from the DLS and from a detailed galaxy redshift survey—the Smithsonian Hectospec Lensing Survey (SHEL…

2014 The Astrophysical Journal
XMM-Newton 8
The Gas-rich Circumbinary Disk of HR 4049. I. A Detailed Study of the Mid-infrared Spectrum
DOI: 10.1088/0004-637X/780/1/41 Bibcode: 2014ApJ...780...41M

Cami, J.; Malek, S. E.

We present a detailed analysis of the mid-infrared spectrum of the peculiar evolved object HR 4049. The full Spitzer-IRS high-resolution spectrum shows a wealth of emission with prominent features from CO2 and H2O and possible contributions from HCN and OH. We model the molecular emission and find that it originates from a ma…

2014 The Astrophysical Journal
ISO 8
The Variable Near-infrared Counterpart of the Microquasar GRS 1758-258
DOI: 10.1088/2041-8205/797/1/L1 Bibcode: 2014ApJ...797L...1L

Luque-Escamilla, Pedro L.; Martí, Josep; Muñoz-Arjonilla, Álvaro J.

We present a new study of the microquasar system GRS 1758-258 in the near-infrared domain based on archival observations with the Hubble Space Telescope and the NICMOS camera. In addition to confirming the near-infrared counterpart pointed out by Muñoz-Arjonilla et al., we show that this object displays significant photometric variability. From it…

2014 The Astrophysical Journal
eHST 8
Energy-dependent Evolution in IC10 X-1: Hard Evidence for an Extended Corona and Implications
DOI: 10.1088/0004-637X/792/2/131 Bibcode: 2014ApJ...792..131B

Steiner, J. F.; Stevens, I. R.; Barnard, R. +3 more

We have analyzed a ~130 ks XMM-Newton observation of the dynamically confirmed black hole + Wolf-Rayet (BH+WR) X-ray binary (XB) IC10 X-1, covering ~1 orbital cycle. This system experiences periodic intensity dips every ~35 hr. We find that energy-independent evolution is rejected at a >5σ level. The spectral and timing evolution of IC10 X-1 ar…

2014 The Astrophysical Journal
XMM-Newton 8
Spectral Lag Features of GRB 060814 from Swift BAT and Suzaku Observations
DOI: 10.1088/0004-637X/782/2/105 Bibcode: 2014ApJ...782..105R

Roychoudhury, Arundhati; Sarkar, Samir K.; Bhadra, Arunava

This work reports a study on the spectral lag of the prompt emission spectrum of a multi-pulse gamma-ray burst (GRB) GRB 060814 (z = 0.84) using the observations of the Swift Burst Alert Telescope and the Suzaku Wide Area Monitor. We found that the spectral lag for GRB 060814 is positive for the first two and the fourth pulses, while the third pul…

2014 The Astrophysical Journal
Suzaku 8
Diagnostics of the Solar Corona from Comparison between Faraday Rotation Measurements and Magnetohydrodynamic Simulations
DOI: 10.1088/0004-637X/789/2/163 Bibcode: 2014ApJ...789..163L

Kasper, J. C.; Cohen, O.; Le Chat, G. +1 more

Polarized natural radio sources passing behind the Sun experience Faraday rotation as a consequence of the electron density and magnetic field strength in coronal plasma. Since Faraday rotation is proportional to the product of the density and the component of the magnetic field along the line of sight of the observer, a model is required to inter…

2014 The Astrophysical Journal
SOHO 8
The Time-dependent Chemistry of Cometary Debris in the Solar Corona
DOI: 10.1088/0004-637X/785/1/50 Bibcode: 2014ApJ...785...50P

Bryans, P.; Pesnell, W. D.

Recent improvements in solar observations have greatly progressed the study of sungrazing comets. They can now be imaged along the entirety of their perihelion passage through the solar atmosphere, revealing details of their composition and structure not measurable through previous observations in the less volatile region of the orbit further from…

2014 The Astrophysical Journal
PROBA-2 8
Initiation and Early Evolution of the Coronal Mass Ejection on 2009 May 13 from Extreme-ultraviolet and White-light Observations
DOI: 10.1088/0004-637X/793/2/140 Bibcode: 2014ApJ...793..140R

Reva, A. A.; Ulyanov, A. S.; Kuzin, S. V. +1 more

We present the results of the observations of a coronal mass ejection (CME) that occurred on 2009 May 13. The most important feature of these observations is that the CME was observed from the very early stage (the solar surface) up to a distance of 15 solar radii (R ). Below 2 R , we used the data from the TESIS extreme-ul…

2014 The Astrophysical Journal
SOHO 8
Initial Results from NuSTAR Observations of the Norma Arm
DOI: 10.1088/0004-637X/791/1/68 Bibcode: 2014ApJ...791...68B

Hailey, Charles J.; Mori, Kaya; Bauer, Franz E. +13 more

Results are presented for an initial survey of the Norma Arm gathered with the focusing hard X-Ray Telescope NuSTAR. The survey covers 0.2 deg2 of sky area in the 3-79 keV range with a minimum and maximum raw depth of 15 ks and 135 ks, respectively. Besides a bright black-hole X-ray binary in outburst (4U 1630-47) and a new X-ray transi…

2014 The Astrophysical Journal
XMM-Newton 8