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Dynamic response of the Martian ionosphere to an interplanetary shock: Mars Express and MAVEN observations
DOI: 10.1002/2017GL074897 Bibcode: 2017GeoRL..44.9116H

Gurnett, D. A.; Halekas, J. S.; Kopf, A. J. +10 more

Multipoint observations from the Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) instrument on board Mars Express and the Mars Atmosphere and Volatile EvolutioN (MAVEN) mission reveal a dynamic response of the Martian ionosphere to abrupt variations in the upstream solar wind plasma. On 2 February 2017, MAVEN, located upstream …

2017 Geophysical Research Letters
MEx 16
Long-Term Variability of Jupiter's Magnetodisk and Implications for the Aurora
DOI: 10.1002/2017JA024066 Bibcode: 2017JGRA..12212090V

Bunce, Emma J.; Clarke, John T.; Vogt, Marissa F. +2 more

Observations of Jupiter's UV auroral emissions collected over several years show that the ionospheric positions of the main emission and the Ganymede footprint can vary by as much as 3° in latitude. One explanation for this shift is a change of Jupiter's current sheet current density, which would alter the amount of field line stretching and displ…

2017 Journal of Geophysical Research (Space Physics)
eHST 16
AGN Activity in Nucleated Galaxies as Measured by Chandra
DOI: 10.3847/1538-4357/aa6d63 Bibcode: 2017ApJ...841...51F

Baldassare, Vivienne F.; Gültekin, Kayhan; Gnedin, Oleg Y. +4 more

Motivated by theoretical expectations that nuclear star clusters (NSCs) in galactic centers may provide a favorable environment for supermassive black holes to form and/or efficiently grow, we set out to measure the fraction of nearby nucleated galaxies that also host an active galactic nucleus. We targeted a distance-limited sample of 98 objects …

2017 The Astrophysical Journal
eHST 16
Characterization of dust aggregates in the vicinity of the Rosetta spacecraft
DOI: 10.1093/mnras/stx1692 Bibcode: 2017MNRAS.469S.312G

Jorda, L.; Lamy, P. L.; Lara, L. M. +49 more

In a Rosetta/OSIRIS imaging activity in 2015 June, we have observed the dynamic motion of particles close to the spacecraft. Due to the focal setting of the OSIRIS wide angle camera, these particles were blurred, which can be used to measure their distances to the spacecraft. We detected 109 dust aggregates over a 130 min long sequence, and find t…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 16
Dust in Clusters: Separating the Contribution of Galaxies and Intracluster Media
DOI: 10.3847/1538-4357/835/1/111 Bibcode: 2017ApJ...835..111G

López-Corredoira, M.; Gutiérrez, C. M.

We have analyzed a sample of 327 clusters of galaxies, spanning the range of 0.06-0.70 in redshift. Strong constraints on their mean intracluster emission of dust have been obtained using maps and catalogs from the Herschel MerMES project; within a radius of 5 arcmin centered in each cluster, the 95% C.L. limits obtained are 86.6, 48.2, and 30.9 m…

2017 The Astrophysical Journal
Herschel 16
A Heuristic Approach to Remove the Background Intensity on White-light Solar Images. I. STEREO/HI-1 Heliospheric Images
DOI: 10.3847/1538-4357/aa6a12 Bibcode: 2017ApJ...839...68S

Stenborg, Guillermo; Howard, Russell A.

White-light coronal and heliospheric imagers observe scattering of photospheric light from both dust particles (the F-Corona) and free electrons in the corona (the K-corona). The separation of the two coronae is thus vitally important to reveal the faint K-coronal structures (e.g., streamers, co-rotating interaction regions, coronal mass ejections…

2017 The Astrophysical Journal
SOHO 16
Constraining C III] Emission in a Sample of Five Luminous z = 5.7 Galaxies
DOI: 10.3847/2041-8213/aa6482 Bibcode: 2017ApJ...838L..22D

Siana, Brian; Fan, Xiaohui; Jiang, Linhua +6 more

Recent observations have suggested that the C III]λ 1907/1909 emission lines could be alternative diagnostic lines for galaxies in the reionization epoch. We use the F128N narrowband filter on the Hubble Space Telescope’s (HST) Wide Field Camera 3 (WFC3) to search for C III] emission in a sample of five galaxies at z = 5.7 in the Subaru Deep Field…

2017 The Astrophysical Journal
eHST 16
Near-Earth plasma sheet boundary dynamics during substorm dipolarization
DOI: 10.1186/s40623-017-0707-2 Bibcode: 2017EP&S...69..129N

Strangeway, Robert J.; Plaschke, Ferdinand; Russell, Christopher T. +29 more

We report on the large-scale evolution of dipolarization in the near-Earth plasma sheet during an intense (AL ~ ‑1000 nT) substorm on August 10, 2016, when multiple spacecraft at radial distances between 4 and 15 RE were present in the night-side magnetosphere. This global dipolarization consisted of multiple short-timescale (a couple o…

2017 Earth, Planets and Space
Cluster 16
Rapid X-ray variability properties during the unusual very hard state in neutron-star low-mass X-ray binaries
DOI: 10.1093/mnras/stx2006 Bibcode: 2017MNRAS.472..559W

Altamirano, D.; Degenaar, N.; Wijnands, R. +2 more

Here, we study the rapid X-ray variability (using XMM-Newton observations) of three neutron-star low-mass X-ray binaries (1RXS J180408.9-342058, EXO 1745-248 and IGR J18245-2452) during their recently proposed very hard spectral state. All our systems exhibit a strong to very strong noise component in their power density spectra (rms amplitudes ra…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 16
Venus's winds and temperatures during the MESSENGER's flyby: An approximation to a three-dimensional instantaneous state of the atmosphere
DOI: 10.1002/2017GL072900 Bibcode: 2017GeoRL..44.3907P

Clancy, R. T.; Hueso, R.; Sánchez-Lavega, A. +14 more

Even though many missions have explored the Venus atmospheric circulation, its instantaneous state is poorly characterized. In situ measurements vertically sampling the atmosphere exist for limited locations and dates, while remote sensing observations provide only global averages of winds at altitudes of the clouds: 47, 60, and 70 km. We present …

2017 Geophysical Research Letters
VenusExpress 16