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Cometary science after Rosetta
DOI: 10.1098/rsta.2017.0001 Bibcode: 2017RSPTA.37570001J

Knight, Matthew M.; Jones, Geraint H.; Fitzsimmons, Alan +1 more

The European Space Agency's Rosetta mission ended operations on 30 September 2016 having spent over 2 years in close proximity to its target comet, 67P/Churyumov-Gerasimenko. Shortly before this, in summer 2016, a discussion meeting was held to examine how the results of the mission could be framed in terms of cometary and solar system science in …

2017 Philosophical Transactions of the Royal Society of London Series A
Rosetta 6
Suzaku observations of spectral variations of the ultra-luminous X-ray source Holmberg IX X-1
DOI: 10.1093/pasj/psw108 Bibcode: 2017PASJ...69....4K

Makishima, Kazuo; Nakazawa, Kazuhiro; Kobayashi, Shogo B.

Observations of the ultra-luminous X-ray source (ULX) Holmberg IX X-1 were carried out with Suzaku twice, once on 2012 April 13 and then on 2012 October 24, with exposures of 180 ks and 217 ks, respectively. The source showed a hard power-law shaped spectrum with a mild cutoff at ∼8 keV, which is typical of ULXs when they are relatively dim. On bo…

2017 Publications of the Astronomical Society of Japan
Suzaku 6
Turbulent processes in Earth's magnetosheath by Cluster mission measurements
DOI: 10.1016/j.jastp.2016.12.016 Bibcode: 2017JASTP.154..115K

Lui, A. T. Y.; Kronberg, E. A.; Kozak, L. V. +1 more

Methods and approaches which can be used for the analysis of hydrodynamic and magnetohydrodynamic turbulent flows are chosen for this study. It is defined that the best methods for determination of turbulent process types are the methods of statistical physics. Within the statistical approach the fractal analysis (height of the maximum of probabil…

2017 Journal of Atmospheric and Solar-Terrestrial Physics
Cluster 6
Multiwavelength observations of the Be/X-ray binary IGR J01217-7257 (=SXP 2.16) during outburst
DOI: 10.1093/mnras/stw3169 Bibcode: 2017MNRAS.466.1149B

Udalski, A.; Coe, M. J.; Bird, A. J. +6 more

We present simultaneous, multiwavelength observations of the Small Magellanic Cloud Be/XRB IGR J01217-7257 (=SXP 2.16) during outbursts in 2014, 2015 and 2016. We also present the results of the RXTE observations of the Small Magellanic Cloud during which the source was initially discovered with a periodicity of 2.1652 ± 0.0001 s that we associate…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 6
Ionospheric Electron Densities at Mars: Comparison of Mars Express Ionospheric Sounding and MAVEN Local Measurements
DOI: 10.1002/2017JA024629 Bibcode: 2017JGRA..12212393N

Gurnett, D. A.; Němec, F.; Morgan, D. D. +5 more

We present the first direct comparison of Martian ionospheric electron densities measured by the Mars Advanced Radar for Subsurface and Ionospheric Sounding (MARSIS) topside radar sounder on board the Mars Express spacecraft and by the Langmuir Probe and Waves (LPW) instrument on board the Mars Atmosphere and Volatile Evolution Mission (MAVEN) spa…

2017 Journal of Geophysical Research (Space Physics)
MEx 6
A Jupiter-mass planet around the K0 giant HD 208897
DOI: 10.1051/0004-6361/201731184 Bibcode: 2017A&A...608A..14Y

Yılmaz, M.; Sato, B.; Bikmaev, I. +9 more

For over 10 years, we have carried out a precise radial velocity (RV) survey to find substellar companions around evolved G, K-type stars to extend our knowledge of planet formation and evolution. We performed high precision RV measurements for the giant star HD 208897 using an iodine (I2) absorption cell. The measure…

2017 Astronomy and Astrophysics
Hipparcos 6
Time Evolution of Elemental Ratios in Solar Energetic Particle Events
DOI: 10.3847/1538-4357/aa5274 Bibcode: 2017ApJ...835...71Z

Dalla, S.; Cohen, C. M. S.; Mewaldt, R. A. +1 more

Heavy ion ratio abundances in solar energetic particle (SEP) events, e.g., Fe/O, often exhibit decreases over time. Using particle instruments on the Advanced Composition Explorer, Solar and Heliospheric Observatory and Solar Terrestrial Relations Observatory spacecraft, we analyzed heavy ion data from 4 SEP events taking place between 2006 Decemb…

2017 The Astrophysical Journal
SOHO 6
De-noising the galaxies in the Hubble XDF with EMPCA
DOI: 10.1093/mnras/stx1380 Bibcode: 2017MNRAS.471..750M

Maturi, Matteo

We present a method to model optical images of galaxies using expectation maximization principal components analysis. The method returns de-noised images, it relies on the data alone and does not assume any pre-established model or fitting formula. It preserves the statistical properties of the sample, minimizing possible biases. The precision of …

2017 Monthly Notices of the Royal Astronomical Society
eHST 6
Just how hot are the ω Centauri extreme horizontal branch pulsators?
DOI: 10.1051/0004-6361/201630132 Bibcode: 2017A&A...600A.130L

Ely, J.; Latour, M.; Chayer, P. +5 more

Context. Past studies based on optical spectroscopy suggest that the five ω Cen pulsators form a rather homogeneous group of hydrogen-rich subdwarf O stars with effective temperatures of around 50 000 K. This places the stars below the red edge of the theoretical instability strip in the log g-Teff diagram, where no p…

2017 Astronomy and Astrophysics
IUE eHST 6
Study of ice-related flow features around Tanaica Montes, Mars: Implications for late amazonian debris-covered glaciation
DOI: 10.1016/j.icarus.2017.07.002 Bibcode: 2017Icar..297..217S

Vijayan, S.; Sinha, Rishitosh K.; Bharti, Rajiv R.

Lobate debris aprons (LDA) and lineated valley fill (LVF) have been broadly recognized in the mid-latitudes of Mars and their subsequent analyses using data from the SHAllow RADar (SHARAD) instrument has suggested evidence for contemporary ice preserved beneath these features. In this study, we conduct detailed characterization of newly identified…

2017 Icarus
MEx 6