Search Publications

An X-ray view of HD 166734, a massive supergiant system
DOI: 10.1051/0004-6361/201630303 Bibcode: 2017A&A...607A..97N

Nazé, Yaël; Mahy, Laurent; Gosset, Eric +1 more

The X-ray emission of the O+O binary HD 166734 was monitored using Swift and XMM-Newton observatories, leading to the discovery of phase-locked variations. The presence of an f line in the He-like triplets further supports a wind-wind collision as the main source of the X-rays in HD 166734. While temperature and absorption do not vary significantl…

2017 Astronomy and Astrophysics
XMM-Newton 8
On the dust and gas components of the z = 2.8 gravitationally lensed quasar host RX J0911.4+0551
DOI: 10.1093/mnras/stx212 Bibcode: 2017MNRAS.467.3513T

Tuan-Anh, P.; Hoai, D. T.; Nhung, P. T. +4 more

Observations by the Atacama Large Millimetre/sub-millimetre Array of the 358 GHz continuum emission of the gravitationally lensed quasar host RX J0911.4+0551 have been analysed. They complement earlier Plateau de Bure Interferometer observations of the CO(7-6) emission. The good knowledge of the lensing potential obtained from the Hubble Space Tel…

2017 Monthly Notices of the Royal Astronomical Society
eHST 8
Origin of Radio Enhancements in Type II Bursts in the Outer Corona
DOI: 10.1007/s11207-017-1148-6 Bibcode: 2017SoPh..292..127A

Valtonen, Eino; Pohjolainen, Silja; Al-Hamadani, Firas

We study interplanetary (IP) solar radio type II bursts from 2011 - 2014 in order to determine the cause of the intense enhancements in their radio emission. Type II bursts are known to be due to propagating shocks that are often associated with fast halo-type coronal mass ejections (CMEs). We analysed the radio spectral data and the white-light c…

2017 Solar Physics
SOHO 8
The role of plasma slowdown in the generation of Rhea's Alfvén wings
DOI: 10.1002/2016JA023595 Bibcode: 2017JGRA..122.1778K

Dougherty, Michele K.; Russell, Christopher T.; Fatemi, Shahab +5 more

Alfvén wings are known to form when a conducting or mass-loading object slows down a flowing plasma in its vicinity. Alfvén wings are not expected to be generated when an inert moon such as Rhea interacts with Saturn's magnetosphere, where the plasma impacting the moon is absorbed and the magnetic flux passes unimpeded through the moon. However, i…

2017 Journal of Geophysical Research (Space Physics)
Cassini 8
2D kinematic study of the central region of NGC 4501
DOI: 10.1093/mnras/stw2275 Bibcode: 2017MNRAS.464..293R

Rodrigues, I.; Repetto, P.; Faúndez-Abans, M. +2 more

Gemini Multi-Object Spectrograph and its Integral Field Unit observational data were used to study the detailed 2D gas kinematics and morphological structures within the ∼500 × 421 pc2 of the active Seyfert 2 galaxy NGC 4501. We provide empirical pieces of evidence of possible outflowing material from the central zones of NGC 4501 to th…

2017 Monthly Notices of the Royal Astronomical Society
eHST 8
On-ground testing of the role of adhesion in the LISA-Pathfinder test mass injection phase
DOI: 10.1016/j.asr.2017.02.030 Bibcode: 2017AdSpR..59.2572B

Bortoluzzi, D.; Zanoni, C.; Conklin, J. W.

Many space missions share the need to fly a free-falling body inside the spacecraft, as a reference for navigation and/or as a probe for the local gravitational field. When a mechanism is required to cage such an object during the launch phase, the need arises to release it to free-fall once the operational phase must be initiated in orbit. The cr…

2017 Advances in Space Research
LISAPathfinder 8
Hubble Space Telescope Ultraviolet Light Curves Reveal Interesting Properties of CC Sculptoris and RZ Leonis
DOI: 10.3847/1538-3881/aa5c88 Bibcode: 2017AJ....153..123S

Szkody, Paula; Sion, Edward M.; Godon, Patrick +6 more

Time-tag ultraviolet data obtained on the Hubble Space Telescope in 2013 reveal interesting variability related to the white dwarf spin in the two cataclysmic variables RZ Leo and CC Scl. RZ Leo shows a period at 220 s and its harmonic at 110 s, thus identifying it as a likely Intermediate Polar (IP). The spin signal is not visible in a short sing…

2017 The Astronomical Journal
eHST 8
Panchromatic spectral energy distributions of simulated galaxies: results at redshift z = 0
DOI: 10.1093/mnras/stx869 Bibcode: 2017MNRAS.469.3775G

Annunziatella, Marianna; Obreja, Aura; Granato, Gian Luigi +5 more

We present predictions of spectral energy distributions (SEDs), from the UV to the FIR, of simulated galaxies at z = 0. These were obtained by post-processing the results of an N-body+hydro simulation of a cosmological box of side 25 Mpc, which uses the Multi-Phase Particle Integrator (MUPPI) for star formation and stellar feedback, with the grasi…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 8
Propagation Characteristics of Two Coronal Mass Ejections from the Sun Far into Interplanetary Space
DOI: 10.3847/1538-4357/aa5ea3 Bibcode: 2017ApJ...837....4Z

Wang, Rui; Liu, Ying D.; Hu, Huidong +1 more

Propagation of coronal mass ejections (CMEs) from the Sun far into interplanetary space is not well understood, due to limited observations. In this study we examine the propagation characteristics of two geo-effective CMEs, which occurred on 2005 May 6 and 13, respectively. Significant heliospheric consequences associated with the two CMEs are ob…

2017 The Astrophysical Journal
SOHO Ulysses 8
Study of the progenitor of the magnetar 1E 2259+586 through Suzaku observations of the associated supernova remnant CTB 109
DOI: 10.1093/pasj/psx012 Bibcode: 2017PASJ...69...40N

Enoto, Teruaki; Makishima, Kazuo; Nakano, Toshio +4 more

We present a study of the progenitor of the magnetar 1E 2259+586, from Suzaku observations of the associated supernova remnant CTB 109. The Suzaku spectra, either spatially integrated or spatially resolved, were successfully described by a two-component plasma model, which reconfirms a previous Chandra result on the northwestern part of this remna…

2017 Publications of the Astronomical Society of Japan
Suzaku 8