Search Publications

Comparison between 2D and 3D Parameters of 306 Front-side Halo CMEs from 2009 to 2013
DOI: 10.3847/0004-637X/821/2/95 Bibcode: 2016ApJ...821...95J

Cho, K. -S.; Moon, Y. -J.; Jang, Soojeong +2 more

We investigate 306 LASCO front-side halo (partial and full) CMEs from 2009 to 2013, which are well-observed by both the Solar and Heliospheric Observatory (SOHO) and the Solar TErrestrial RElations Observatory (STEREO). These CMEs have two-dimensional (2D) parameters, such as speed, angular width, and propagation direction, from a single spacecraf…

2016 The Astrophysical Journal
SOHO 23
X-ray, UV and optical analysis of supergiants: ɛ Ori
DOI: 10.1093/mnras/stv2783 Bibcode: 2016MNRAS.456.2907P

Hillier, D. John; Leutenegger, Maurice A.; Cohen, David H. +2 more

We present a multi-wavelength (X-ray to optical) analysis, based on non-local thermodynamic equilibrium photospheric+wind models, of the B0 Ia-supergiant: ɛ Ori. The aim is to test the consistency of physical parameters, such as the mass-loss rate and CNO abundances, derived from different spectral bands. The derived mass-loss rate is {dot {M}} / …

2016 Monthly Notices of the Royal Astronomical Society
IUE XMM-Newton eHST 23
No Evidence of Intrinsic Optical/Near-infrared Linear Polarization for V404 Cygni during Its Bright Outburst in 2015: Broadband Modeling and Constraint on Jet Parameters
DOI: 10.3847/0004-637X/823/1/35 Bibcode: 2016ApJ...823...35T

Morokuma, T.; Cheung, C. C.; Fukazawa, Y. +39 more

We present simultaneous optical and near-infrared (NIR) polarimetric results for the black hole binary V404 Cyg spanning the duration of its seven-day-long optically brightest phase of its 2015 June outburst. The simultaneous R- and K s -band light curves showed almost the same temporal variation except for the isolated (∼30-minute dur…

2016 The Astrophysical Journal
INTEGRAL 23
Evolution of the X-Ray Properties of the Transient Magnetar XTE J1810-197
DOI: 10.3847/0004-637X/818/2/122 Bibcode: 2016ApJ...818..122A

Halpern, J. P.; Alford, J. A. J.

We report on X-ray observations of the 5.54 s transient magnetar XTE J1810-197 using the XMM-Newton and Chandra observatories, analyzing new data from 2008 through 2014, and re-analyzing data from 2003 through 2007 with the benefit of these six years of new data. From the discovery of XTE J1810-197 during its 2003 outburst to the most recent 2014 …

2016 The Astrophysical Journal
XMM-Newton 23
Temporal Gain Correction for X-ray Calorimeter Spectrometers
DOI: 10.1007/s10909-016-1503-2 Bibcode: 2016JLTP..184..498P

Tsujimoto, M.; Ishisaki, Y.; Yamada, S. +14 more

Calorimetric X-ray detectors are very sensitive to their environment. The boundary conditions can have a profound effect on the gain including heat sink temperature, the local radiation temperature, bias, and the temperature of the readout electronics. Any variation in the boundary conditions can cause temporal variations in the gain of the detect…

2016 Journal of Low Temperature Physics
Hitomi 23
Ne X X-ray emission due to charge exchange in M82
DOI: 10.1093/mnras/stw527 Bibcode: 2016MNRAS.458.3554C

Liu, L.; Cumbee, R. S.; Lyons, D. +4 more

Recent X-ray observations of star-forming galaxies such as M82 have shown the Ly β/Ly α line ratio of Ne X to be in excess of predictions for thermal electron impact excitation. Here, we demonstrate that the observed line ratio may be due to charge exchange and can be used to constrain the ion kinetic energy to be ≲ 500 eV/u. This is accomplished …

2016 Monthly Notices of the Royal Astronomical Society
Suzaku 23
SAPS onset timing during substorms and the westward traveling surge
DOI: 10.1002/2016GL069693 Bibcode: 2016GeoRL..43.6687M

Mishin, Evgeny, V.

We present multispacecraft observations in the magnetosphere and conjugate ionosphere of the onset time of subauroral polarization streams (SAPS) and tens of keV ring current injections on the duskside in three individual substorms. This is probably the first unequivocal determination of the substorm SAPS onset timing. The time lag between the SAP…

2016 Geophysical Research Letters
Cluster 23
X-ray/UV variability and the origin of soft X-ray excess emission from II Zw 177
DOI: 10.1093/mnras/stw009 Bibcode: 2016MNRAS.457..875P

Dewangan, Gulab C.; Pal, Main; Misra, Ranjeev +1 more

We study X-ray and UV emission from the narrow-line Seyfert 1 galaxy II Zw 177 using a 137 ks long and another 13 ks short XMM-Newton observation performed in 2012 and 2001, respectively. Both observations show soft X-ray excess emission contributing 76.9 ± 4.9 per cent in 2012 and 58.8 ± 10.2 per cent in 2001 in the 0.3-2 keV band. We find that b…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 23
Evidence for a 36 ks phase modulation in the hard X-ray pulses from the magnetar 1E 1547.0-5408
DOI: 10.1093/pasj/psv097 Bibcode: 2016PASJ...68S..12M

Enoto, Teruaki; Makishima, Kazuo; Nakazawa, Kazuhiro +4 more

The Suzaku data for the highly variable magnetar 1E 1547.0-5408, obtained during the 2009 January activity, were reanalyzed. The 2.07 s pulsation, detected in the 15-40 keV HXD data, was found to exhibit phase modulation, which can be modeled by a sinusoid with a period of 36.0^{+4.5}_{-2.5}ks and an amplitude of 0.52 ± 0.14 s. While the effect is…

2016 Publications of the Astronomical Society of Japan
Suzaku 23
Hydrological and sedimentary analyses of well-preserved paleofluvial-paleolacustrine systems at Moa Valles, Mars
DOI: 10.1002/2015JE004891 Bibcode: 2016JGRE..121..194S

Hauber, Ernst; Di Achille, Gaetano; Ori, Gian Gabriele +2 more

Moa Valles is a well-preserved, likely Amazonian (younger than 2 Ga old), paleodrainage system that is nearly 300 km long and carved into ancient highland terrains west of Idaeus Fossae. The fluvial system apparently originated from fluidized ejecta blankets, and it consists of a series of dam breach paleolakes with associated fan-shaped sedimenta…

2016 Journal of Geophysical Research (Planets)
MEx 23