Search Publications

An Evolutionary Study of Volatile Chemistry in Protoplanetary Disks
DOI: 10.3847/1538-4357/ab9e71 Bibcode: 2020ApJ...898...97B

Wilner, David J.; Cleeves, L. Ilsedore; Andrews, Sean M. +11 more

The volatile composition of a planet is determined by the inventory of gas and ice in the parent disk. The volatile chemistry in the disk is expected to evolve over time, though this evolution is poorly constrained observationally. We present Atacama Large Millimeter/submillimeter Array observations of C18O, C2H, and the isot…

2020 The Astrophysical Journal
Gaia 53
Shadowing and multiple rings in the protoplanetary disk of HD 139614
DOI: 10.1051/0004-6361/201936509 Bibcode: 2020A&A...635A.121M

Ménard, F.; Matter, A.; Henning, T. +20 more

Context. Shadows in scattered light images of protoplanetary disks are a common feature and support the presence of warps or misalignments between disk regions. These warps are possibly caused by an inclined (sub-)stellar companion embedded in the disk.
Aims: We aim to study the morphology of the protoplanetary disk around the Herbig Ae star …

2020 Astronomy and Astrophysics
Gaia 53
A Very Young Radio-loud Magnetar
DOI: 10.3847/2041-8213/ab9742 Bibcode: 2020ApJ...896L..30E

Campana, S.; Tiengo, A.; Götz, D. +20 more

The magnetar Swift J1818.0-1607 was discovered in 2020 March when Swift detected a 9 ms hard X-ray burst and a long-lived outburst. Prompt X-ray observations revealed a spin period of 1.36 s, soon confirmed by the discovery of radio pulsations. We report here on the analysis of the Swift burst and follow-up X-ray and radio observations. The burst …

2020 The Astrophysical Journal
XMM-Newton 53
The magnetic field and accretion regime of CI Tau
DOI: 10.1093/mnras/stz3368 Bibcode: 2020MNRAS.491.5660D

Moutou, C.; Ménard, F.; Donati, J. -F. +7 more

This paper exploits spectropolarimetric data of the classical T Tauri star CI Tau collected with ESPaDOnS at the Canada-France-Hawaii Telescope, with the aims of detecting and characterizing the large-scale magnetic field that the star hosts, and of investigating how the star interacts with the inner regions of its accretion disc through this fiel…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 53
Lithium in red giant stars: Constraining non-standard mixing with large surveys in the Gaia era
DOI: 10.1051/0004-6361/201936360 Bibcode: 2020A&A...633A..34C

Jasniewicz, G.; Lagarde, N.; Smiljanic, R. +7 more

Context. Li is extensively known to be a good tracer of non-standard mixing processes occurring in stellar interiors.
Aims: We present the results of a new large Li survey in red giant stars and combine it with surveys from the literature to probe the impact of rotation-induced mixing and thermohaline double-diffusive instability along stella…

2020 Astronomy and Astrophysics
Gaia Hipparcos 53
High-resolution Spectroscopy of the GD-1 Stellar Stream Localizes the Perturber near the Orbital Plane of Sagittarius
DOI: 10.3847/2041-8213/ab800c Bibcode: 2020ApJ...892L..37B

Conroy, Charlie; Cargile, Phillip A.; Johnson, Benjamin D. +6 more

The 100° long thin stellar stream in the Milky Way halo, GD-1, has an ensemble of features that may be due to dynamical interactions. Using high-resolution MMT/Hectochelle spectroscopy we show that a spur of GD-1-like stars outside of the main stream are kinematically and chemically consistent with the main stream. In the spur, as in the main stre…

2020 The Astrophysical Journal
Gaia 53
Refining the age, emplacement and alteration scenarios of the olivine-rich unit in the Nili Fossae region, Mars
DOI: 10.1016/j.icarus.2019.113436 Bibcode: 2020Icar..33613436M

Mangold, N.; Quantin-Nataf, C.; Millot, C. +8 more

The Nili Fossae region of Mars exhibits from remote sensing spectral data the largest exposures of olivine-rich materials on the planet. However, it is not clearly constrained how and when these terrains formed. Some of the proposed scenarios favor a mode of formation closely related to Isidis impact basin: either under intense effusive volcanism …

2020 Icarus
MEx 53
Keck Observations Confirm a Super-Jupiter Planet Orbiting M Dwarf OGLE-2005-BLG-071L
DOI: 10.3847/1538-3881/ab6212 Bibcode: 2020AJ....159...68B

Lu, Jessica R.; Cole, Andrew A.; Udalski, Andrzej +10 more

We present adaptive optics imaging from the NIRC2 instrument on the Keck II telescope that resolves the exoplanet host (and lens) star as it separates from the brighter source star. These observations yield the K-band brightness of the lens and planetary host star, as well as the lens-source relative proper motion, ${{\boldsymbol{\mu }}}_{\mathrm{…

2020 The Astronomical Journal
Gaia eHST 52
Obliquity Constraints on an Extrasolar Planetary-mass Companion
DOI: 10.3847/1538-3881/ab76c6 Bibcode: 2020AJ....159..181B

Knutson, Heather A.; Morley, Caroline V.; Bowler, Brendan P. +8 more

We place the first constraints on the obliquity of a planetary-mass companion outside of the solar system. Our target is the directly imaged system 2MASS J01225093-2439505 (2M0122), which consists of a 120 Myr 0.4 M star hosting a 12-27 MJ companion at 50 au. We constrain all three of the system's angular-momentum vectors: h…

2020 The Astronomical Journal
Gaia eHST 52
GOODS-ALMA: The slow downfall of star formation in z = 2-3 massive galaxies
DOI: 10.1051/0004-6361/202038312 Bibcode: 2020A&A...643A..30F

Magnelli, B.; Daddi, E.; Elbaz, D. +34 more

We investigate the properties of a sample of 35 galaxies, detected with the Atacama Large Millimeter/Submillimeter Array (ALMA) at 1.1 mm in the GOODS-ALMA field (area of 69 arcmin2, resolution = 0.60″, rms ≃ 0.18 mJy beam-1). Using the ultraviolet-to-radio deep multiwavelength coverage of the GOODS-South field, we fit the sp…

2020 Astronomy and Astrophysics
Herschel eHST 52