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Machine-learning Regression of Extinction in the Second Gaia Data Release
DOI: 10.3847/1538-3881/ab63d5 Bibcode: 2020AJ....159...84B

Bai, Yu; Wang, Song; Liu, JiFeng +1 more

Machine learning has become a popular tool to help us make better decisions and predictions, based on experiences, observations, and analyzing patterns, within a given data set without explicit functions. In this paper, we describe an application of the supervised machine-learning algorithm to the extinction regression for the second Gaia data rel…

2020 The Astronomical Journal
Gaia 8
Subaru Near-infrared Imaging Polarimetry of Misaligned Disks around the SR 24 Hierarchical Triple System
DOI: 10.3847/1538-3881/ab5850 Bibcode: 2020AJ....159...12M

Henning, Thomas; Nakagawa, Takao; Terada, Hiroshi +66 more

The SR 24 multistar system hosts both circumprimary and circumsecondary disks, which are strongly misaligned with each other. The circumsecondary disk is circumbinary in nature. Interestingly, both disks are interacting, and they possibly rotate in opposite directions. To investigate the nature of this unique twin disk system, we present 0.″1 reso…

2020 The Astronomical Journal
Gaia 8
Calibrating the Galactic Cepheid Period-Luminosity Relation from the Maximum-likelihood Technique
DOI: 10.3847/1538-3881/aba627 Bibcode: 2020AJ....160..136L

Lazovik, Yaroslav A.; Rastorguev, Alexey S.

We present a realization of the maximum-likelihood technique, which is one of the latest modifications of the Baade-Becker-Wesselink method. Our approach is based on nonlinear calibrations of the effective temperature and bolometric correction, which take into account metallicity and surface gravity. It allows one to estimate the key Cepheid param…

2020 The Astronomical Journal
Gaia 8
Visual Orbits of Spectroscopic Binaries with the CHARA Array. III. HD 8374 and HD 24546
DOI: 10.3847/1538-3881/ab8f95 Bibcode: 2020AJ....160...58L

Gies, Douglas R.; Lester, Kathryn V.; Monnier, John D. +9 more

We present the visual orbits of two long-period spectroscopic binary stars, HD 8374 and HD 24546, using interferometric observations acquired with the CHARA Array and the Palomar Testbed Interferometer. We also obtained new radial velocities from echelle spectra using the APO 3.5 m and Fairborn 2.0 m telescopes. By combining the visual and spectro…

2020 The Astronomical Journal
Gaia 8
Robustly Detecting Changes in Warm Jupiters' Transit Impact Parameters
DOI: 10.3847/1538-3881/ab7fa5 Bibcode: 2020AJ....159..223D

Dawson, Rebekah I.

Torques from a mutually inclined perturber can change a transiting planet's impact parameter, resulting in variations in the transit shape and duration. Detection of and upper limits on changes in impact parameter yield valuable constraints on a planetary system's three-dimensional architecture. Constraints for warm Jupiters are particularly inter…

2020 The Astronomical Journal
Gaia 7
Discovery of a Nearby Young Brown Dwarf Disk
DOI: 10.3847/1538-3881/abaccd Bibcode: 2020AJ....160..156S

Debes, John H.; Kiman, Rocio; Schneider, Adam C. +16 more

We report the discovery of the youngest brown dwarf with a disk at 102 pc from the Sun, WISEA J120037.79-784508.3 (W1200-7845), via the Disk Detective citizen science project. We establish that W1200-7845 is located in the ${3.7}_{-1.4}^{+4.6}$ Myr old ɛ Cha association. Its spectral energy distribution (SED) exhibits clear evidence of an infrared…

2020 The Astronomical Journal
Gaia 7
A Wide-orbit Exoplanet OGLE-2012-BLG-0838Lb
DOI: 10.3847/1538-3881/ab8a49 Bibcode: 2020AJ....159..261P

Soszyński, I.; Udalski, A.; Szymański, M. K. +50 more

We present the discovery of a planet on a very wide orbit in the microlensing event OGLE-2012-BLG-0838. The signal of the planet is well separated from the main peak of the event and the planet-star projected separation is found to be twice the Einstein ring radius, which corresponds to a projected separation of ≈4 au. Similar planets around low-m…

2020 The Astronomical Journal
Gaia 7
Magnetic Inflation and Stellar Mass. V. Intensification and Saturation of M-dwarf Absorption Lines with Rossby Number
DOI: 10.3847/1538-3881/ab5d3d Bibcode: 2020AJ....159...52M

Muirhead, Philip S.; Mann, Andrew W.; Newton, Elisabeth R. +2 more

In young Sun-like stars and field M-dwarf stars, chromospheric and coronal magnetic activity indicators such as Hα, X-ray, and radio emission are known to saturate with low Rossby number (Ro ≲ 0.1), defined as the ratio of rotation period to convective turnover time. The mechanism for the saturation is unclear. In this paper, we use photospheric T…

2020 The Astronomical Journal
Gaia 7
A High Angular Resolution Survey of Massive Stars in Cygnus OB2: JHK Adaptive Optics Results from the Gemini Near-Infrared Imager
DOI: 10.3847/1538-3881/aba536 Bibcode: 2020AJ....160..115C

Goodwin, S. P.; Gies, D. R.; ten Brummelaar, T. A. +8 more

We present results of a high angular resolution survey of massive OB stars in the Cygnus OB2 association that we conducted with the Near-Infrared Imager camera and ALTAIR adaptive optics system of the Gemini North telescope. We observed 74 O- and early-B-type stars in Cyg OB2 in the JHK infrared bands in order to detect binary and multiple compani…

2020 The Astronomical Journal
eHST 7
A Search for Polarized Thermal Emission from Directly Imaged Exoplanets and Brown Dwarf Companions to Nearby Stars
DOI: 10.3847/1538-3881/abc33d Bibcode: 2020AJ....160..286J

Jensen-Clem, Rebecca; De Rosa, Robert J.; Hinkley, Sasha +15 more

Aerosols in the atmospheres of cloudy gas giant exoplanets and brown dwarfs scatter and polarize these objects' thermal emission. If such an object has an oblate shape or nonuniform cloud distribution, the net degree of linear polarization can show an increase ranging from several tenths of a percent to a few percent. Modern high-contrast imaging …

2020 The Astronomical Journal
Gaia 7