Search Publications

Double Stars and Astrometric Uncertainties in Gaia DR1
DOI: 10.3847/2041-8213/aa6af1 Bibcode: 2017ApJ...840L...1M

Makarov, Valeri V.; Frouard, Julien; Fabricius, Claus

A significant number of double stars with separations up to 2.5 arcsec are present in the Gaia Data Release 1 astrometric catalogs. Limiting our analysis to a well-studied sample of 1124 doubles resolved by Hipparcos, provided with individual Tycho component photometry and cross-matched with the TGAS catalog, we estimate a rate of at least 3% for …

2017 The Astrophysical Journal
Gaia Hipparcos 8
Constraining the break of spatial diffeomorphism invariance with Planck data
DOI: 10.1088/1475-7516/2017/07/013 Bibcode: 2017JCAP...07..013G

Alcaniz, J. S.; Graef, L. L.; Benetti, M.

The current most accepted paradigm for the early universe cosmology, the inflationary scenario, shows a good agreement with the recent Cosmic Microwave Background (CMB) and polarization data. However, when the inflation consistency relation is relaxed, these observational data exclude a larger range of red tensor tilt values, prevailing the blue o…

2017 Journal of Cosmology and Astroparticle Physics
Planck 8
Mutated hybrid inflation on brane and reheating temperature
DOI: 10.1140/epjp/i2017-11575-8 Bibcode: 2017EPJP..132..303F

Ferricha-Alami, M.; Sakhi, Z.; Chakir, H. +1 more

In the mutated hybrid-inflation standard case, the spectral index ns is constrained by the e-folds number N, and the gravitational waves are negligible (

2017 European Physical Journal Plus
Planck 8
SPIN: An Inversion Code for the Photospheric Spectral Line
DOI: 10.1007/s11207-017-1131-2 Bibcode: 2017SoPh..292..105Y

Mathew, Shibu K.; Yadav, Rahul; Tiwary, Alok Ranjan

Inversion codes are the most useful tools to infer the physical properties of the solar atmosphere from the interpretation of Stokes profiles. In this paper, we present the details of a new Stokes Profile INversion code (SPIN) developed specifically to invert the spectro-polarimetric data of the Multi-Application Solar Telescope (MAST) at Udaipur …

2017 Solar Physics
Hinode 8
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