Search Publications

Bayesian Characterization of Main-sequence Binaries in the Old Open Cluster NGC 188
DOI: 10.3847/1538-3881/ab59d7 Bibcode: 2020AJ....159...11C

Cohen, Roger E.; von Hippel, Ted; Geller, Aaron M.

The binary fractions of open and globular clusters yield powerful constraints on their dynamical state and evolutionary history. We apply publicly available Bayesian analysis tools to a UBV RIJHK S photometric catalog of the open cluster NGC 188 to detect and characterize photometric binaries along the cluster main sequence. This tech…

2020 The Astronomical Journal
Gaia 15
Statistics of Wide Pre-main-sequence Binaries in the Orion OB1 Association
DOI: 10.3847/1538-3881/abc2d6 Bibcode: 2020AJ....160..268T

Tokovinin, Andrei; Petr-Gotzens, Monika G.; Briceño, Cesar

Statistics of low-mass pre-main-sequence binaries in the Orion OB1 association with separations ranging from 0"6 to 20″ (220 to 7400 au at 370 pc) are studied using images from the VISTA Orion mini survey and astrometry from Gaia. The input sample based on the CVSO catalog contains 1137 stars of K and M spectral types (masses between 0.3 and 0.9 $…

2020 The Astronomical Journal
Gaia 15
Multiple Explanations for the Single Transit of KIC 5951458 Based on Radial Velocity Measurements Extracted with a Novel Matched-template Technique
DOI: 10.3847/1538-3881/abad27 Bibcode: 2020AJ....160..149D

Kane, Stephen R.; Howard, Andrew W.; Dalba, Paul A. +2 more

Planetary systems that show single-transit events are a critical pathway to increasing the yield of long-period exoplanets from transit surveys. From the primary Kepler mission, KIC 5951458 b (Kepler-456b) was thought to be a single-transit giant planet with an orbital period of 1310 days. However, radial velocity (RV) observations of KIC 5951458 …

2020 The Astronomical Journal
Gaia 15
Observations of Disintegrating Long-period Comet C/2019 Y4 (ATLAS): A Sibling of C/1844 Y1 (Great Comet)
DOI: 10.3847/1538-3881/ab9d81 Bibcode: 2020AJ....160...91H

Ye, Quan-Zhi; Hui, Man-To

We present a study of C/2019 Y4 (ATLAS) using Sloan gri observations from 2020 mid-January to early April. During this time span, the comet brightened with a growth in the effective cross-section of $\left(2.0\pm 0.1\right)\times {10}^{2}$ m2 s-1 from the beginning to ∼70 days preperihelion in late 2020 March, followed by a b…

2020 The Astronomical Journal
Gaia 15
An Analysis of the Statistics and Systematics of Limb Anomaly Detections in HST/STIS Transit Images of Europa
DOI: 10.3847/1538-3881/ab7454 Bibcode: 2020AJ....159..155G

Strobel, Darrell; Saur, Joachim; Giono, Gabriel +5 more

Several recent studies derived the existence of plumes on Jupiter's moon Europa. The only technique that provided multiple detections is the far-ultraviolet imaging observations of Europa in transit of Jupiter taken by the Space Telescope Imaging Spectrograph (STIS) on the Hubble Space Telescope (HST). In this study, we reanalyze the three HST/STI…

2020 The Astronomical Journal
eHST 15
Hubble Space Telescope Search for Activity in High-perihelion Objects
DOI: 10.3847/1538-3881/ab7faf Bibcode: 2020AJ....159..209L

Mutchler, Max; Jewitt, David; Agarwal, Jessica +2 more

Solar system objects with perihelia beyond the orbit of Jupiter (q > 5 au) are too cold for water ice to generate an appreciable coma via sublimation. Despite this, numerous high-perihelion objects (HPOs) including many comets and recently escaped Kuiper Belt objects (Centaurs) are observed to be active out at least to the orbit of Saturn (q ∼ …

2020 The Astronomical Journal
eHST 15
Beyond Gaia: Asteroseismic Distances of M Giants Using Ground-based Transient Surveys
DOI: 10.3847/1538-3881/ab91bf Bibcode: 2020AJ....160...18A

Kochanek, C. S.; Huber, Daniel; Tonry, John +14 more

Evolved stars near the tip of the red giant branch show solar-like oscillations with periods spanning hours to months and amplitudes ranging from ∼1 mmag to ∼100 mmag. The systematic detection of the resulting photometric variations with ground-based telescopes would enable the application of asteroseismology to a much larger and more distant samp…

2020 The Astronomical Journal
Gaia 15
HD 150382: A Lithium-rich Star at the Early-AGB Stage?
DOI: 10.3847/1538-3881/ab5528 Bibcode: 2020AJ....159....9H

Pereira, C. B.; Holanda, N.; Drake, N. A.

We report the discovery of a lithium-rich giant, HD 150382, a post-red-giant-branch clump star. The atmospheric parameters, the chemical abundances for 17 elements, and the isotopic ratio 12C/13C were determined using the equivalent width and the spectral synthesis methods. The lithium abundance was determined via spectral sy…

2020 The Astronomical Journal
Gaia 15
Upper Limits on Planet Occurrence around Ultracool Dwarfs with K2
DOI: 10.3847/1538-3881/ab9224 Bibcode: 2020AJ....160...19S

Muirhead, Philip S.; Sagear, Sheila A.; Skinner, Julie N.

The occurrence of planets orbiting ultracool dwarfs is poorly constrained. We present results from a guest observer program on NASA's K2 spacecraft to search for transiting planets orbiting a sample of 827 ultracool dwarfs. Having found no transiting planets in our sample, we determined an upper limit on the occurrence of planets. We simulated pla…

2020 The Astronomical Journal
Gaia 14
Orbital Motion, Variability, and Masses in the T Tauri Triple System
DOI: 10.3847/1538-3881/ab93be Bibcode: 2020AJ....160...35S

Prato, L.; Schaefer, G. H.; Beck, Tracy L. +1 more

We present results from adaptive optics imaging of the T Tauri triple system obtained at the Keck and Gemini Observatories in 2015-2019. We fit the orbital motion of T Tau Sb relative to Sa and model the astrometric motion of their center of mass relative to T Tau N. Using the distance measured by Gaia, we derived dynamical masses of ${M}_{\mathrm…

2020 The Astronomical Journal
Gaia 14