Search Publications

Spatial variations of brightness, colour and polarization of dust in comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stx2003 Bibcode: 2017MNRAS.469S.475R

Afanasiev, Viktor L.; Rosenbush, Vera K.; Ivanova, Oleksandra V. +2 more

We present post-perihelion photometric and polarimetric observations of comet 67P/Churyumov-Gerasimenko performed at the 6-m telescope of the SAO RAS in the g-sdss (465/65 nm), r-sdss (620/60 nm) and R filters. Observations in November and December 2015 and April 2016 covered the range of heliocentric distance 1.62-2.72 au and phase angle 33.2°-10…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 43
Quiescent Prominence Dynamics Observed with the Hinode Solar Optical Telescope. II. Prominence Bubble Boundary Layer Characteristics and the Onset of a Coupled Kelvin-Helmholtz Rayleigh-Taylor Instability
DOI: 10.3847/1538-4357/aa95b6 Bibcode: 2017ApJ...850...60B

Liu, Wei; Hillier, Andrew; Berger, Thomas

We analyze solar quiescent prominence bubble characteristics and instability dynamics using Hinode/Solar Optical Telescope data. We measure the bubble expansion rate, prominence downflows, and the profile of the boundary layer brightness and thickness as a function of time. The largest bubble analyzed rises into the prominence with a speed of abou…

2017 The Astrophysical Journal
Hinode 43
Not that long time ago in the nearest galaxy: 3D slice of molecular gas revealed by a 110 yr old flare of Sgr A*
DOI: 10.1093/mnras/stw2750 Bibcode: 2017MNRAS.465...45C

Sunyaev, R.; Churazov, E.; Ponti, G. +1 more

A powerful outburst of X-ray radiation from the supermassive black hole Sgr A* at the centre of the Milky Way is believed to be responsible for the illumination of molecular clouds in the central ∼100 pc of the Galaxy (Sunyaev, Markevitch & Pavlinsky; Koyama et al.). The reflected/reprocessed radiation comes to us with a delay corresponding to…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 43
Multitracer CMB delensing maps from Planck and WISE data
DOI: 10.1103/PhysRevD.96.123511 Bibcode: 2017PhRvD..96l3511Y

Sherwin, Blake D.; Hill, J. Colin; Yu, Byeonghee

Delensing, the removal of the limiting lensing B -mode background, is crucial for the success of future cosmic microwave background (CMB) surveys in constraining inflationary gravitational waves (IGWs). In recent work, delensing with large-scale structure tracers has emerged as a promising method both for improving constraints on IGWs and for test…

2017 Physical Review D
Planck 43
NOMAD spectrometer on the ExoMars trace gas orbiter mission: part 2—design, manufacturing, and testing of the ultraviolet and visible channel
DOI: 10.1364/ao.56.002771 Bibcode: 2017ApOpt..56.2771P

Vandaele, Ann Carine; Neefs, Eddy; Ristic, Bojan +48 more

2017 Applied Optics
ExoMars-16 43
Dwarf nova outbursts in intermediate polars
DOI: 10.1051/0004-6361/201730760 Bibcode: 2017A&A...602A.102H

Hameury, J. -M.; Lasota, J. -P.

Context. The disc instability model (DIM) has been very successful in explaining the dwarf nova outbursts observed in cataclysmic variables. When, as in intermediate polars, the accreting white dwarf is magnetised, the disc is truncated at the magnetospheric radius, but for mass-transfer rates corresponding to the thermal-viscous instability such …

2017 Astronomy and Astrophysics
Gaia 42
Topographic Constraints on the Evolution and Connectivity of Titan's Lacustrine Basins
DOI: 10.1002/2017GL075468 Bibcode: 2017GeoRL..4411745H

Lorenz, R. D.; Hayes, A. G.; Kirk, R. L. +11 more

The topography provided by altimetry, synthetic aperture radar-topography, and stereo radargrammetry has opened new doors for Titan research by allowing for quantitative analysis of morphologic form. Using altimetry measurements, we show that Titan's Maria are consistent with an equipotential surface but that several filled lakes are found to be h…

2017 Geophysical Research Letters
Cassini 42
The VIMOS Ultra-Deep Survey: A major merger origin for the high fraction of galaxies at 2 < z < 6 with two bright clumps
DOI: 10.1051/0004-6361/201630057 Bibcode: 2017A&A...608A..16R

Maccagni, D.; Schaerer, D.; Koekemoer, A. +12 more

The properties of stellar clumps in star-forming galaxies and their evolution over the redshift range 2 ≲ z ≲ 6 are presented and discussed in the context of the build-up of massive galaxies at early cosmic times. We focused on galaxies with spectroscopic redshifts from the VIMOS Ultra Deep Survey (VUDS) and stellar masses log 10(M

2017 Astronomy and Astrophysics
eHST 42
Capacitive sensing of test mass motion with nanometer precision over millimeter-wide sensing gaps for space-borne gravitational reference sensors
DOI: 10.1103/PhysRevD.96.062004 Bibcode: 2017PhRvD..96f2004A

Mendes, L.; Madden, S.; Russano, G. +100 more

We report on the performance of the capacitive gap-sensing system of the Gravitational Reference Sensor on board the LISA Pathfinder spacecraft. From in-flight measurements, the system has demonstrated a performance, down to 1 mHz, that is ranging between 0.7 and 1.8 aF Hz-1 /2 . That translates into a sensing noise of the test mass mot…

2017 Physical Review D
LISAPathfinder 42
Spatially resolved evolution of the local H2O production rates of comet 67P/Churyumov-Gerasimenko from the MIRO instrument on Rosetta
DOI: 10.1051/0004-6361/201730502 Bibcode: 2017A&A...603A..87M

Ip, W. -H.; Hartogh, P.; Lellouch, E. +11 more


Aims: Using spectroscopic and continuum data measured by the MIRO instrument on board Rosetta of comet 67P/Churyumov-Gerasimenko, it is possible to derive and track the change in the water production rate, to learn how the outgassing evolves with heliocentric distance. The MIRO data are well suited to investigate the evolution of 67P, in unpr…

2017 Astronomy and Astrophysics
Rosetta 42