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Improved measurements of turbulence in the hot gaseous atmospheres of nearby giant elliptical galaxies
DOI: 10.1093/mnras/stx2030 Bibcode: 2017MNRAS.472.1659O

Kaastra, J. S.; de Plaa, J.; Fabian, A. C. +7 more

We present significantly improved measurements of turbulent velocities in the hot gaseous haloes of nearby giant elliptical galaxies. Using deep XMM-Newton Reflection Grating Spectrometer (RGS) observations and a combination of resonance scattering and direct line broadening methods, we obtain well bounded constraints for 13 galaxies. Assuming tha…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 68
Change of outgassing pattern of 67P/Churyumov-Gerasimenko during the March 2016 equinox as seen by ROSINA
DOI: 10.1093/mnras/stx1412 Bibcode: 2017MNRAS.469S.108G

Mall, Urs; De Keyser, Johan; Berthelier, Jean-Jacques +18 more

As the spin axis of comet 67P/Churyumov-Gerasimenko (67P) is not normal to the orbital plane, 67P has strong seasonal changes in the illumination conditions on the nucleus' surface, with a short and intense summer in the Southern hemisphere. We have been monitoring these seasonal variations in the gas coma with the Rosetta Orbiter Spectrometer for…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 68
The Carnegie-Chicago Hubble Program. II. The Distance to IC 1613: The Tip of the Red Giant Branch and RR Lyrae Period-luminosity Relations
DOI: 10.3847/1538-4357/aa7f73 Bibcode: 2017ApJ...845..146H

Madore, Barry F.; Freedman, Wendy L.; Beaton, Rachael L. +8 more

IC 1613 is an isolated dwarf galaxy within the Local Group. Low foreground and internal extinction, low metallicity, and low crowding make it an invaluable testbed for the calibration of the local distance ladder. We present new, high-fidelity distance estimates to IC 1613 via its Tip of the Red Giant Branch (TRGB) and its RR Lyrae (RRL) variables…

2017 The Astrophysical Journal
Gaia eHST 68
D2O and HDS in the coma of 67P/Churyumov-Gerasimenko
DOI: 10.1098/rsta.2016.0253 Bibcode: 2017RSPTA.37560253A

Altwegg, K.; Balsiger, H.; Berthelier, J. J. +12 more

The European Rosetta mission has been following comet 67P/Churyumov-Gerasimenko for 2 years, studying the nucleus and coma in great detail. For most of these 2 years the Rosetta Orbiter Sensor for Ion and Neutral Analysis (ROSINA) has analysed the volatile part of the coma. With its high mass resolution and sensitivity it was able to not only dete…

2017 Philosophical Transactions of the Royal Society of London Series A
Rosetta 68
Orbiting Clouds of Material at the Keplerian Co-rotation Radius of Rapidly Rotating Low-mass WTTs in Upper Sco
DOI: 10.3847/1538-3881/aa5eb9 Bibcode: 2017AJ....153..152S

Pinsonneault, Marc; Cody, Ann Marie; Rebull, Luisa +8 more

Using K2 data, we identified 23 very-low-mass members of the ρ Oph and Upper Scorpius star-forming region as having periodic photometric variability not easily explained by well-established physical mechanisms such as star spots, eclipsing binaries, or pulsation. All of these unusual stars are mid-to-late M dwarfs without evidence of active accret…

2017 The Astronomical Journal
AKARI Gaia 68
Comet 67P outbursts and quiescent coma at 1.3 au from the Sun: dust properties from Rosetta/VIRTIS-H observations
DOI: 10.1093/mnras/stx1950 Bibcode: 2017MNRAS.469S.443B

Mottola, S.; Erard, S.; Crovisier, J. +15 more

We present 2-5 µm spectroscopic observations of the dust coma of 67P/Churyumov-Gerasimenko obtained with the VIRTIS-H instrument onboard Rosetta during two outbursts that occurred on 2015, 13 September 13.6 h ut and 14 September 18.8 h ut at 1.3 au from the Sun. Scattering and thermal properties measured before the outburst are in the mean o…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 68
No evidence for Population III stars or a Direct Collapse Black Hole in the z = 6.6 Lyman-α emitter 'CR7'
DOI: 10.1093/mnras/stx839 Bibcode: 2017MNRAS.469..448B

Bowler, R. A. A.; McLure, R. J.; Dunlop, J. S. +4 more

The z = 6.6 Lyman α emitter 'CR7' has been claimed to have a Population III (Pop III) like stellar population, or alternatively, be a candidate direct collapse black hole (DCBH). In this paper, we investigate the evidence for these exotic scenarios using recently available, deeper, optical, near-infrared and mid-infrared imaging. We find strong Sp…

2017 Monthly Notices of the Royal Astronomical Society
eHST 68
Cosmological discordances: A new measure, marginalization effects, and application to geometry versus growth current data sets
DOI: 10.1103/PhysRevD.96.023532 Bibcode: 2017PhRvD..96b3532L

Ishak, Mustapha; Lin, Weikang

The continuous progress toward more precise cosmological surveys and experiments has galvanized recent interest into consistency tests on cosmological parameters and models. At the heart of this effort is quantifying the degree of inconsistency between two or more cosmological data sets. We introduce an intuitive moment-based measure we call the i…

2017 Physical Review D
Planck 68
The life cycles of Be viscous decretion discs: time-dependent modelling of infrared continuum observations
DOI: 10.1093/mnras/stw2542 Bibcode: 2017MNRAS.464.3071V

Carciofi, A. C.; Rivinius, Th.; Vieira, R. G. +3 more

We apply the viscous decretion disc (VDD) model to interpret the infrared disc continuum emission of 80 Be stars observed in different epochs. In this way, we determined 169 specific disc structures, namely their density scale, ρ0, and exponent, n. We found that the n values range mainly between 1.5 and 3.5, and ρ0 varies bet…

2017 Monthly Notices of the Royal Astronomical Society
AKARI 68
The ALMA Frontier Fields Survey. I. 1.1 mm continuum detections in Abell 2744, MACS J0416.1-2403 and MACS J1149.5+2223
DOI: 10.1051/0004-6361/201628806 Bibcode: 2017A&A...597A..41G

Kneissl, R.; Demarco, R.; Treister, E. +21 more

Context. Dusty star-forming galaxies are among the most prodigious systems at high redshift (z > 1), characterized by high star-formation rates and huge dust reservoirs. The bright end of this population has been well characterized in recent years, but considerable uncertainties remain for fainter dusty star-forming galaxies, which are responsi…

2017 Astronomy and Astrophysics
eHST 68