Search Publications

Kinematics of OB-associations in Gaia epoch
DOI: 10.1093/mnras/stx2225 Bibcode: 2017MNRAS.472.3887M

Dambis, A. K.; Mel'nik, A. M.

We use stellar proper motions from the Tycho-Gaia Astrometric Solution (TGAS) catalogue to study the kinematics of OB-associations. The TGAS proper motions of OB-associations generally agree well with the Hipparcos proper motions. The parameters of the Galactic rotation curve obtained with TGAS and Hipparcos proper motions agree within the errors.…

2017 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 56
The search for multiple populations in Magellanic Cloud clusters - I. Two stellar populations in the Small Magellanic Cloud globular cluster NGC 121
DOI: 10.1093/mnras/stw2269 Bibcode: 2017MNRAS.464...94N

Dalessandro, E.; Salaris, M.; Larsen, S. +14 more

We started a photometric survey using the WFC3/UVIS instrument onboard the Hubble Space Telescope to search for multiple populations within Magellanic Cloud star clusters at various ages. In this paper, we introduce this survey. As first results of this programme, we also present multiband photometric observations of NGC 121 in different filters t…

2017 Monthly Notices of the Royal Astronomical Society
eHST 56
On a New Theoretical Framework for RR Lyrae Stars. II. Mid-infrared Period-Luminosity-Metallicity Relations
DOI: 10.3847/1538-4357/aa713d Bibcode: 2017ApJ...841...84N

Madore, Barry F.; Freedman, Wendy L.; Beaton, Rachael L. +14 more

We present new theoretical period-luminosity-metallicity (PLZ) relations for RR Lyræ stars (RRLs) at Spitzer and WISE wavelengths. The PLZ relations were derived using nonlinear, time-dependent convective hydrodynamical models for a broad range of metal abundances (Z = 0.0001-0.0198). In deriving the light curves, we tested two sets of atmospheric…

2017 The Astrophysical Journal
Gaia 56
BICEP2 / Keck Array IX: New bounds on anisotropies of CMB polarization rotation and implications for axionlike particles and primordial magnetic fields
DOI: 10.1103/PhysRevD.96.102003 Bibcode: 2017PhRvD..96j2003B

Ade, P. A. R.; Bock, J. J.; Crill, B. P. +64 more

We present the strongest constraints to date on anisotropies of cosmic microwave background (CMB) polarization rotation derived from 150 GHz data taken by the BICEP2 & Keck Array CMB experiments up to and including the 2014 observing season (BK14). The definition of the polarization angle in BK14 maps has gone through self-calibration in which…

2017 Physical Review D
Planck 56
A centrally heated dark halo for our Galaxy
DOI: 10.1093/mnras/stw2775 Bibcode: 2017MNRAS.465..798C

Binney, James; Cole, D. R.

We construct a new family of models of our Galaxy in which dark matter and disc stars are both represented by distribution functions that are analytic functions of the action integrals of motion. The potential that is self-consistently generated by the dark matter, stars, and gas is determined, and parameters in the distribution functions are adju…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 56
The black hole binary V404 Cygni: a highly accreting obscured AGN analogue
DOI: 10.1093/mnras/stx466 Bibcode: 2017MNRAS.468..981M

Motta, S. E.; Sánchez-Fernández, C.; Kuulkers, E. +2 more

Typical black hole binaries in outburst show spectral states and transitions, characterized by a clear connection between the inflow on to the black hole and outflows from its vicinity. The transient stellar mass black hole binary V404 Cyg apparently does not fit in this picture. Its outbursts are characterized by intense flares and intermittent p…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 56
The SOFIA Massive (SOMA) Star Formation Survey. I. Overview and First Results
DOI: 10.3847/1538-4357/aa74c8 Bibcode: 2017ApJ...843...33D

Tanaka, Kei E. I.; Zhang, Yichen; Tan, Jonathan C. +6 more

We present an overview and first results of the Stratospheric Observatory For Infrared Astronomy Massive (SOMA) Star Formation Survey, which is using the FORCAST instrument to image massive protostars from ∼10 to 40 µm. These wavelengths trace thermal emission from warm dust, which in Core Accretion models mainly emerges from the inner regio…

2017 The Astrophysical Journal
Herschel 56
A test of Gaia Data Release 1 parallaxes: implications for the local distance scale
DOI: 10.1051/0004-6361/201629733 Bibcode: 2017A&A...599A..67C

Casertano, Stefano; Riess, Adam G.; Bucciarelli, Beatrice +1 more


Aims: We present a comparison of Gaia Data Release 1 (DR1) parallaxes with photometric parallaxes for a sample of 212 Galactic Cepheids at a median distance of 2 kpc, and explore their implications on the distance scale and the local value of the Hubble constant H0.
Methods: The Cepheid distances are estimated from a recent ca…

2017 Astronomy and Astrophysics
Gaia 56
The lensing and temperature imprints of voids on the cosmic microwave background
DOI: 10.1093/mnras/stw3299 Bibcode: 2017MNRAS.466.3364C

Cai, Yan-Chuan; Neyrinck, Mark; Mao, Qingqing +3 more

We have searched for the signature of cosmic voids in the cosmic microwave background (CMB), in both the Planck temperature and lensing-convergence maps; voids should give decrements in both. We use ZOBOV voids from the Data Release 12 Sloan Digital Sky Survey CMASS galaxy sample. We base our analysis on N-body simulations, to avoid a posteriori b…

2017 Monthly Notices of the Royal Astronomical Society
Planck 56
Cosmological parameters, shear maps and power spectra from CFHTLenS using Bayesian hierarchical inference
DOI: 10.1093/mnras/stw3161 Bibcode: 2017MNRAS.466.3272A

Jaffe, Andrew H.; Heavens, Alan; Alsing, Justin

We apply two Bayesian hierarchical inference schemes to infer shear power spectra, shear maps and cosmological parameters from the Canada-France-Hawaii Telescope (CFHTLenS) weak lensing survey - the first application of this method to data. In the first approach, we sample the joint posterior distribution of the shear maps and power spectra by Gib…

2017 Monthly Notices of the Royal Astronomical Society
Planck 56