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Multi-wavelength properties of IGR J05007-7047 (LXP 38.55) and identification as a Be X-ray binary pulsar in the LMC
DOI: 10.1093/mnras/stw1408 Bibcode: 2016MNRAS.461.1875V

Haberl, F.; Udalski, A.; Sturm, R. +2 more

We report on the results of a ∼40-d multi-wavelength monitoring of the Be X-ray binary system IGR J05007-7047 (LXP 38.55). During that period the system was monitored in the X-rays using the Swift telescope and in the optical with multiple instruments. When the X-ray luminosity exceeded 1036 erg s-1 we triggered an XMM-Newton…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 17
Coalescence of magnetic flux ropes observed in the tailward high-speed flows
DOI: 10.1002/2016JA023526 Bibcode: 2016JGRA..12110898Z

Zhao, Yan; Yao, Zhonghua; Lu, Quanming +3 more

We report a tailward high-speed flow event observed by Cluster during 0203:00UT-0205:30UT on 20 September 2003. Within the flows, a series of three bipolar Bz signatures were observed. The first and third bipolar Bz signatures are identified as magnetic flux ropes, while the middle one is found to result from the collision of…

2016 Journal of Geophysical Research (Space Physics)
Cluster 17
Constraints on the H2O formation mechanism in the wind of carbon-rich AGB stars
DOI: 10.1051/0004-6361/201527049 Bibcode: 2016A&A...588A.124L

Blommaert, J. A. D. L.; De Ridder, J.; de Koter, A. +13 more

Context. The recent detection of warm H2O vapor emission from the outflows of carbon-rich asymptotic giant branch (AGB) stars challenges the current understanding of circumstellar chemistry. Two mechanisms have been invoked to explain warm H2O vapor formation. In the first, periodic shocks passing through the medium immediate…

2016 Astronomy and Astrophysics
Herschel ISO 17
The size and shape of the Milky Way disc and halo from M-type brown dwarfs in the BoRG survey
DOI: 10.1093/mnras/stw258 Bibcode: 2016MNRAS.458..425V

Trenti, M.; Bouwens, R. J.; Holwerda, B. W. +3 more

We have identified 274 M-type brown dwarfs in the Hubble Space Telescope's Wide Field Camera 3 pure parallel fields from the Brightest of Reionizing Galaxies (BoRG) survey for high-redshift galaxies. These are near-infrared observations with multiple lines of sight out of our Milky Way. Using these observed M-type brown dwarfs, we fitted a Galacti…

2016 Monthly Notices of the Royal Astronomical Society
eHST 17
The Secret Lives of Cepheids: Evolution, Mass-Loss, and Ultraviolet Emission of the Long-period Classical Cepheid
DOI: 10.3847/0004-637X/824/1/1 Bibcode: 2016ApJ...824....1N

Guinan, Edward F.; Engle, Scott G.; Neilson, Hilding R. +2 more

The classical Cepheid l Carinae is an essential calibrator of the Cepheid Leavitt Law as a rare long-period Galactic Cepheid. Understanding the properties of this star will also constrain the physics and evolution of massive (M ≥ 8 M ) Cepheids. The challenge, however, is precisely measuring the star's pulsation period and its rate of …

2016 The Astrophysical Journal
XMM-Newton eHST 17
Flux and spectral variability of the blazar PKS 2155 -304 with XMM-Newton: Evidence of particle acceleration and synchrotron cooling
DOI: 10.1016/j.newast.2015.08.005 Bibcode: 2016NewA...44...21B

Bhagwan, Jai; Papadakis, I. E.; Wiita, Paul J. +1 more

We have analyzed XMM-Newton observations of the high energy peaked blazar, PKS 2155 -304, made on 24 May 2002 in the 0.3-10 keV X-ray band. These observations display a mini-flare, a nearly constant flux period and a strong flux increase. We performed a time-resolved spectral study of the data, by dividing the data into eight segments. We fitted t…

2016 New Astronomy
XMM-Newton 17
Hybrid simulation of Titan's interaction with the supersonic solar wind during Cassini's T96 flyby
DOI: 10.1002/2015GL066848 Bibcode: 2016GeoRL..43...35F

Simon, Sven; Motschmann, Uwe; Neubauer, Fritz M. +5 more

By applying a hybrid (kinetic ions and fluid electrons) simulation code, we study the plasma environment of Saturn's largest moon Titan during Cassini's T96 flyby on 1 December 2013. The T96 encounter marks the only observed event of the entire Cassini mission where Titan was located in the supersonic solar wind in front of Saturn's bow shock. Our…

2016 Geophysical Research Letters
Cassini 17
Source region and growth analysis of narrowband Z-mode emission at Saturn
DOI: 10.1002/2016JA022913 Bibcode: 2016JGRA..12111929M

Gurnett, D. A.; Coates, A. J.; Santolík, O. +5 more

Intense Z-mode emission is observed in the lower density region near the inner edge of the Enceladus torus at Saturn, where these waves may resonate with MeV electrons. The source mechanism of this emission, which is narrow-banded and most intense near 5 kHz, is not well understood. We survey the Cassini Radio and Plasma Wave Science data to isola…

2016 Journal of Geophysical Research (Space Physics)
Cassini 17
Shadowing and anisotropy of solar energetic ions at Mars measured by MAVEN during the March 2015 solar storm
DOI: 10.1002/2015JA022327 Bibcode: 2016JGRA..121.2818L

Lee, Christina O.; Larson, Davin; Halekas, Jasper S. +4 more

The Solar Energetic Particle (SEP) Instrument on the Mars Atmosphere and Volatile EvolutioN (MAVEN) spacecraft is meant to characterize the variability of SEP fluxes at Mars. SEP ion precipitation is an important source of heating, ionization, and chemical changes in the upper atmosphere of Mars and may have played a substantial role in driving at…

2016 Journal of Geophysical Research (Space Physics)
VenusExpress 17
A Chandra Study of Temperature Distributions of the Intracluster Medium in 50 Galaxy Clusters
DOI: 10.3847/0004-637X/816/2/54 Bibcode: 2016ApJ...816...54Z

Hu, Dan; Xu, Haiguang; Zhu, Zhenghao +10 more

To investigate the spatial distribution of the intracluster medium temperature in galaxy clusters in a quantitative way and probe the physics behind it, we analyze the X-ray spectra from a sample of 50 clusters that were observed with the Chandra ACIS instrument over the past 15 years and measure the radial temperature profiles out to 0.45r50…

2016 The Astrophysical Journal
Suzaku 17