Search Publications

High-energy monitoring of NGC 4593 with XMM-Newton and NuSTAR. X-ray spectral analysis
DOI: 10.1093/mnras/stw2022 Bibcode: 2016MNRAS.463..382U

Bianchi, S.; Cappi, M.; Ponti, G. +8 more

We present results from a joint XMM-Newton/NuSTAR monitoring of the Seyfert 1 NGC 4593, consisting of 5 × 20 ks simultaneous observations spaced by 2 d, performed in 2015 January. The source is variable, both in flux and spectral shape, on time-scales down to a few ks and with a clear softer-when-brighter behaviour. In agreement with past observat…

2016 Monthly Notices of the Royal Astronomical Society
XMM-Newton 41
CME impact on comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stw2112 Bibcode: 2016MNRAS.462S..45E

Glassmeier, K. -H.; Behar, E.; Möstl, C. +23 more

We present Rosetta observations from comet 67P/Churyumov-Gerasimenko during the impact of a coronal mass ejection (CME). The CME impacted on 2015 Oct 5-6, when Rosetta was about 800 km from the comet nucleus, and 1.4 au from the Sun. Upon impact, the plasma environment is compressed to the level that solar wind ions, not seen a few days earlier wh…

2016 Monthly Notices of the Royal Astronomical Society
Rosetta SOHO 41
A Hubble Space Telescope Study of the Enigmatic Milky Way Halo Globular Cluster Crater*
DOI: 10.3847/0004-637X/822/1/32 Bibcode: 2016ApJ...822...32W

Dolphin, Andrew E.; Sills, Alison; Belokurov, Vasily +6 more

We analyze the resolved stellar populations of the faint stellar system, Crater, based on deep optical imaging taken with the Advanced Camera for Surveys on the Hubble Space Telescope. Crater’s color-magnitude diagram (CMD) extends ∼4 mag below the oldest main-sequence (MS) turnoff. Structurally, we find that Crater has a half-light radius of ∼20 …

2016 The Astrophysical Journal
eHST 41
NuSTAR and XMM-Newton Observations of the Neutron Star X-Ray Binary 1RXS J180408.9-34205
DOI: 10.3847/0004-637X/824/1/37 Bibcode: 2016ApJ...824...37L

Harrison, F. A.; Fabian, A. C.; Miller, J. M. +8 more

We report on observations of the neutron star (NS) residing in the low-mass X-ray binary 1RXS J180408.9-34205 taken 2015 March by NuSTAR and XMM-Newton while the source was in the hard spectral state. We find multiple reflection features (Fe {{{K}}}α detected with NuSTAR; N vii, O vii, and O viii detected in the RGS) from different ion…

2016 The Astrophysical Journal
XMM-Newton 41
Acetylene on Titan’s Surface
DOI: 10.3847/0004-637X/828/1/55 Bibcode: 2016ApJ...828...55S

Le Mouélic, S.; Cornet, T.; Rodriguez, S. +6 more

Titan’s atmosphere is opaque in the near-infrared due to gaseous absorptions, mainly by methane, and scattering by aerosols, except in a few “transparency windows.” Thus, the composition of Titan’s surface remains difficult to access from space and is still poorly constrained. Photochemical models suggest that most of the organic compounds formed …

2016 The Astrophysical Journal
Cassini 40
Origin of low proton-to-electron temperature ratio in the Earth's plasma sheet
DOI: 10.1002/2016JA022874 Bibcode: 2016JGRA..121.9985G

Zelenyi, L. M.; Sauvaud, J. -A.; Lavraud, B. +4 more

We study the proton-to-electron temperature ratio (Tp/Te) in the plasma sheet (PS) of the Earth's magnetotail using 5 years of Cluster observations (2001-2005). The PS intervals are searched within a region defined with -19 < X ≤ -7 RE and |Y| < 15 RE (GSM) under the condition |BX| ≤ 10 …

2016 Journal of Geophysical Research (Space Physics)
Cluster 40
Variegation of comet 67P/Churyumov-Gerasimenko in regions showing activity
DOI: 10.1051/0004-6361/201527369 Bibcode: 2016A&A...586A..80O

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

Aims.We carried out an investigation of the surface variegation of comet 67P/Churyumov-Gerasimenko, the detection of regions showing activity, the determination of active and inactive surface regions of the comet with spectral methods, and the detection of fallback material.
Methods: We analyzed multispectral data generated with Optical, Spec…

2016 Astronomy and Astrophysics
Rosetta 40
New Parallaxes and a Convergence Analysis for the TW Hya Association
DOI: 10.3847/1538-4357/833/1/95 Bibcode: 2016ApJ...833...95D

Faherty, J. K.; Weinberger, A. J.; Gagné, J. +3 more

The TW Hya Association (TWA) is a nearby stellar association with an age of ∼5-10 Myr. This is an important age for studying the late stages of star and planet formation. We measure the parallaxes of 14 candidate members of TWA. That brings to 38 the total number of individual stars with fully measured kinematics, I.e., proper motion, radial veloc…

2016 The Astrophysical Journal
Gaia 40
Gamma-ray emission from SN2014J near maximum optical light
DOI: 10.1051/0004-6361/201526941 Bibcode: 2016A&A...588A..67I

Sunyaev, R.; Churazov, E.; Hernanz, M. +17 more

Context. The optical light curve of Type Ia supernovae (SNIa) is powered by thermalized gamma-rays produced by the decay of 56Ni and 56Co, the main radioactive isotopes synthesized by the thermonuclear explosion of a C/O white dwarf.
Aims: Gamma-rays escaping the ejecta can be used as a diagnostic tool for studying the c…

2016 Astronomy and Astrophysics
INTEGRAL 40
Global Gradients for Cosmic-Ray Protons in the Heliosphere During the Solar Minimum of Cycle 23/24
DOI: 10.1007/s11207-016-0945-7 Bibcode: 2016SoPh..291.2181V

Potgieter, M. S.; Vos, E. E.

Global gradients for cosmic-ray (CR) protons in the heliosphere are computed with a comprehensive modulation model for the recent prolonged solar minimum of Cycle 23/24. Fortunately, the PAMELA (Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics) and Ulysses/KET (Kiel Electron Telescope) instruments simultaneously observed pro…

2016 Solar Physics
Ulysses 40