Search Publications

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
The Ages and Masses of a Million Galactic-disk Main-sequence Turnoff and Subgiant Stars from the LAMOST Galactic Spectroscopic Surveys
DOI: 10.3847/1538-4365/aa80e4 Bibcode: 2017ApJS..232....2X

Shi, Jianrong; Wu, Yaqian; Xiang, Maosheng +10 more

We present estimates of stellar age and mass for 0.93 million Galactic-disk main-sequence turnoff and subgiant stars from the LAMOST Galactic Spectroscopic Surveys. The ages and masses are determined by matching with stellar isochrones using a Bayesian algorithm, utilizing effective temperature {T}{eff}, absolute magnitude {M}V

2017 The Astrophysical Journal Supplement Series
Gaia 68
Observing the Sun with the Atacama Large Millimeter/submillimeter Array (ALMA): High-Resolution Interferometric Imaging
DOI: 10.1007/s11207-017-1095-2 Bibcode: 2017SoPh..292...87S

de Gregorio-Monsalvo, I.; Kim, S.; De Pontieu, B. +25 more

Observations of the Sun at millimeter and submillimeter wavelengths offer a unique probe into the structure, dynamics, and heating of the chromosphere; the structure of sunspots; the formation and eruption of prominences and filaments; and energetic phenomena such as jets and flares. High-resolution observations of the Sun at millimeter and submil…

2017 Solar Physics
IRIS 68
The Circum-Galactic Medium of Massive Spirals. II. Probing the Nature of Hot Gaseous Halo around the Most Massive Isolated Spiral Galaxies
DOI: 10.3847/1538-4365/aa96fc Bibcode: 2017ApJS..233...20L

Bregman, Joel N.; Anderson, Michael E.; Crain, Robert A. +3 more

We present the analysis of the XMM-Newton data of the Circum-Galactic Medium of MASsive Spirals (CGM-MASS) sample of six extremely massive spiral galaxies in the local universe. All the CGM-MASS galaxies have diffuse X-ray emission from hot gas detected above the background extending ∼ (30{--}100) {kpc} from the galactic center. This doubles the e…

2017 The Astrophysical Journal Supplement Series
XMM-Newton 68
The global mass functions of 35 Galactic globular clusters: I. Observational data and correlations with cluster parameters
DOI: 10.1093/mnras/stx1856 Bibcode: 2017MNRAS.471.3668S

Baumgardt, H.; Sollima, A.

We have derived the global mass functions of a sample of 35 Galactic globular clusters (GCs) by comparing deep Hubble Space Telescope photometry from the globular clusters treasury project (Sarajedini et al. 2007) with suitable multimass dynamical models. For a subset of 29 clusters with available radial velocity information, we were also able to …

2017 Monthly Notices of the Royal Astronomical Society
eHST 67