Search Publications

Constraining the properties of HD 206893 B. A combination of radial velocity, direct imaging, and astrometry data
DOI: 10.1051/0004-6361/201935044 Bibcode: 2019A&A...627L...9G

Aigrain, S.; Rouan, D.; Meunier, N. +25 more

Context. High contrast imaging enables the determination of orbital parameters for substellar companions (planets, brown dwarfs) from the observed relative astrometry and the estimation of model and age-dependent masses from their observed magnitudes or spectra. Combining astrometric positions with radial velocity gives direct constraints on the o…

2019 Astronomy and Astrophysics
Gaia Hipparcos 33
Multispacecraft Analysis of Electron Holes
DOI: 10.1029/2018GL080757 Bibcode: 2019GeoRL..46...55S

Russell, C. T.; Vaivads, A.; Khotyaintsev, Yu. V. +4 more

Electron holes (EHs) are nonlinear electrostatic structures in plasmas. Most previous in situ studies of EHs have been limited to single- and two-spacecraft methods. We present statistics of EHs observed by Magnetospheric Multiscale on the magnetospheric side of the magnetopause during October 2016 when the spacecraft separation was around 6 km. E…

2019 Geophysical Research Letters
Cluster 33
Investigating ULX accretion flows and cyclotron resonance in NGC 300 ULX1
DOI: 10.1051/0004-6361/201834144 Bibcode: 2019A&A...621A.118K

Haberl, F.; Buchner, J.; Vasilopoulos, G. +2 more


Aims: We investigate accretion models for the newly discovered pulsating ultraluminous X-ray source (ULX) NGC 300 ULX1.
Methods: We analyzed broadband XMM-Newton and NuSTAR observations of NGC 300 ULX1, performing phase-averaged and phase-resolved spectroscopy. Using the Bayesian framework, we compared two physically motivated models for…

2019 Astronomy and Astrophysics
XMM-Newton 33
The VMC survey - XXXIV. Morphology of stellar populations in the Magellanic Clouds
DOI: 10.1093/mnras/stz2400 Bibcode: 2019MNRAS.490.1076E

Girardi, Léo; de Grijs, Richard; Ripepi, Vincenzo +11 more

The Magellanic Clouds are nearby dwarf irregular galaxies whose morphologies show different properties when traced by different stellar populations, making them an important laboratory for studying galaxy morphologies. We study the morphology of the Magellanic Clouds using data from the Visible and Infrared Survey Telescope for Astronomy survey of…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 33
From Scattered-light to Millimeter Emission: A Comprehensive View of the Gigayear-old System of HD 202628 and its Eccentric Debris Ring
DOI: 10.3847/1538-3881/ab3ec1 Bibcode: 2019AJ....158..162F

Hughes, A. Meredith; Wilner, David J.; Stapelfeldt, Karl R. +13 more

We present here new observations of the eccentric debris ring surrounding the Gyr-old solar-type star HD 202628: at millimeter wavelengths with ALMA, at far-infrared wavelengths with Herschel, and in scattered light with the Hubble Space Telescope (HST). The ring inner edge is found to be consistent between ALMA and HST data. As radiation pressure…

2019 The Astronomical Journal
Gaia Herschel eHST 33
Prolonged sub-luminous state of the new transitional pulsar candidate CXOU J110926.4‑650224
DOI: 10.1051/0004-6361/201834835 Bibcode: 2019A&A...622A.211C

Rea, Nanda; Coti Zelati, Francesco; Torres, Diego F. +12 more

We report on a multi-wavelength study of the unclassified X-ray source CXOU J110926.4‑650224 (J1109). We identified the optical counterpart as a blue star with a magnitude of ∼20.1 (3300–10500 Å). The optical emission was variable on timescales from hundreds to thousands of seconds. The spectrum showed prominent emission lines with variable profil…

2019 Astronomy and Astrophysics
Gaia INTEGRAL XMM-Newton 33
Revealing the cosmic evolution of boxy/peanut-shaped bulges from HST COSMOS and SDSS
DOI: 10.1093/mnras/stz2877 Bibcode: 2019MNRAS.490.4721K

Debattista, Victor P.; Erwin, Peter; Lintott, Chris +1 more

Vertically thickened bars, observed in the form of boxy/peanut (B/P) bulges, are found in the majority of massive barred disc galaxies in the local Universe, including our own. B/P bulges indicate that their host bars have suffered violent bending instabilities driven by anisotropic velocity distributions. We investigate for the first time how the…

2019 Monthly Notices of the Royal Astronomical Society
eHST 33
Measuring the local matter density using Gaia DR2
DOI: 10.1051/0004-6361/201834718 Bibcode: 2019A&A...623A..30W

Widmark, A.


Aims: We determine the total dynamical matter density in the solar neighbourhood using the second Gaia data release (DR2).
Methods: The dynamical matter density distribution is inferred in a framework of a Bayesian hierarchical model, which accounts for position and velocity of all individual stars, as well as the full error covariance m…

2019 Astronomy and Astrophysics
Gaia 33
K2-264: a transiting multiplanet system in the Praesepe open cluster
DOI: 10.1093/mnras/sty3464 Bibcode: 2019MNRAS.484....8L

Cochran, William D.; Endl, Michael; Tamura, Motohide +31 more

Planet host stars with well-constrained ages provide a rare window to the time domain of planet formation and evolution. The NASA K2 mission has enabled the discovery of the vast majority of known planets transiting stars in clusters, providing a valuable sample of planets with known ages and radii. We present the discovery of two planets transiti…

2019 Monthly Notices of the Royal Astronomical Society
Gaia 33
On the usefulness of existing solar wind models for pulsar timing corrections
DOI: 10.1093/mnras/stz1278 Bibcode: 2019MNRAS.487..394T

Dettmar, R. -J.; Kramer, M.; Zucca, P. +15 more

Dispersive delays due to the solar wind introduce excess noise in high-precision pulsar timing experiments, and must be removed in order to achieve the accuracy needed to detect, e.g., low-frequency gravitational waves. In current pulsar timing experiments, this delay is usually removed by approximating the electron density distribution in the sol…

2019 Monthly Notices of the Royal Astronomical Society
SOHO 33