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Cloud Atlas: Hubble Space Telescope Near-infrared Spectral Library of Brown Dwarfs, Planetary-mass Companions, and Hot Jupiters
DOI: 10.3847/1538-3881/aaf88f Bibcode: 2019AJ....157..101M

Schneider, Glenn; Apai, Dániel; Burgasser, Adam J. +12 more

Bayesian atmospheric retrieval tools can place constraints on the properties of brown dwarfs' and hot Jupiters' atmospheres. To fully exploit these methods, high signal-to-noise spectral libraries with well-understood uncertainties are essential. We present a high signal-to-noise spectral library (1.10-1.69 µm) of the thermal emission of 76 …

2019 The Astronomical Journal
Gaia eHST 37
Stellar Proper Motions in the Orion Nebula Cluster
DOI: 10.3847/1538-3881/aafb09 Bibcode: 2019AJ....157..109K

Lu, Jessica R.; Anderson, Jay; Morris, Mark R. +5 more

The Orion Nebula Cluster (ONC) is the nearest site of ongoing massive star formation, which allows us to study the kinematics and dynamics of the region in detail and constrain star formation theories. Using HST ACS/WFPC2/WFC3IR and Keck II NIRC2 data, we have measured the proper motions of 701 stars within an ∼6‧ × 6‧ field of view around the cen…

2019 The Astronomical Journal
Gaia eHST 37
Long-term Variations of Venus’s 365 nm Albedo Observed by Venus Express, Akatsuki, MESSENGER, and the Hubble Space Telescope
DOI: 10.3847/1538-3881/ab3120 Bibcode: 2019AJ....158..126L

Marcq, Emmanuel; Imamura, Takeshi; Titov, Dmitrij V. +16 more

An unknown absorber near the cloud-top level of Venus generates a broad absorption feature from the ultraviolet (UV) to visible, peaking around 360 nm, and therefore plays a critical role in the solar energy absorption. We present a quantitative study of the variability of the cloud albedo at 365 nm and its impact on Venus’s solar heating rates ba…

2019 The Astronomical Journal
VenusExpress eHST 36
Kinematics of the Palomar 5 Stellar Stream from RR Lyrae Stars
DOI: 10.3847/1538-3881/ab4cef Bibcode: 2019AJ....158..223P

Price-Whelan, Adrian M.; Belokurov, Vasily; Bonaca, Ana +3 more

Thin stellar streams, formed from the tidal disruption of globular clusters, are important gravitational tools, sensitive to both global and small-scale properties of dark matter. The Palomar 5 stellar stream (Pal 5) is an exemplar stream within the Milky Way: its ∼20° tidal tails connect back to the progenitor cluster, and the stream has been use…

2019 The Astronomical Journal
Gaia 36
The Role of Cluster Mass in the Multiple Populations of Galactic and Extragalactic Globular Clusters
DOI: 10.3847/1538-3881/ab45f2 Bibcode: 2019AJ....158..202L

Milone, Antonino P.; Tailo, Marco; Lagioia, Edoardo P. +2 more

Studies based on Hubble Space Telescope (HST) photometry in F275W, F336W, and F438W have shown that the incidence and complexity of multiple populations (MPs) in globular clusters (GCs) depend on cluster mass. This result, however, is based on nearby, low-reddening Galactic GCs, for which we can obtain accurate F275W photometry. In this work, we e…

2019 The Astronomical Journal
Gaia eHST 36
Extreme Debris Disk Variability: Exploring the Diverse Outcomes of Large Asteroid Impacts During the Era of Terrestrial Planet Formation
DOI: 10.3847/1538-3881/ab1260 Bibcode: 2019AJ....157..202S

Reichart, D. E.; Rujopakarn, W.; Dong, Ruobing +14 more

The most dramatic phases of terrestrial planet formation are thought to be oligarchic and chaotic growth, on timescales of up to 100-200 Myr, when violent impacts occur between large planetesimals of sizes up to protoplanets. Such events are marked by the production of large amounts of debris, as has been observed in some exceptionally bright and …

2019 The Astronomical Journal
Gaia 35
Speckle Interferometry at SOAR in 2018
DOI: 10.3847/1538-3881/ab24e4 Bibcode: 2019AJ....158...48T

Tokovinin, Andrei; Briceño, Cesar; Horch, Elliott P. +2 more

The results of speckle interferometric observations at the 4.1 m Southern Astrophysical Research Telescope (SOAR) in 2018 are given, totaling 3097 measurements of 2427 resolved pairs with separations from 11 mas to 5.″9 (median 0.″15, magnitude difference up to 7 mag) and nonresolutions of 624 targets. This work continues our long-term speckle pro…

2019 The Astronomical Journal
Gaia Hipparcos 35
WISE J072003.20-084651.2B is a Massive T Dwarf
DOI: 10.3847/1538-3881/ab3cd1 Bibcode: 2019AJ....158..174D

Shappee, B. J.; Dupuy, Trent J.; Mann, Andrew W. +21 more

We present individual dynamical masses for the nearby M9.5+T5.5 binary WISE J072003.20-084651.2AB, a.k.a. Scholz’s star. Combining high-precision Canada-France-Hawaii Telescope/WIRCam photocenter astrometry and Keck adaptive optics resolved imaging, we measure the first high-quality parallactic distance ({6.80}-0.06+0.05 pc) …

2019 The Astronomical Journal
Gaia 35
Col-OSSOS: Color and Inclination Are Correlated throughout the Kuiper Belt
DOI: 10.3847/1538-3881/aaf72e Bibcode: 2019AJ....157...94M

Wang, Shiang-Yu; Marsset, Michaël; Fraser, Wesley C. +12 more

Both physical and dynamical properties must be considered to constrain the origins of the dynamically excited distant solar system populations. We present high-precision (g-r) colors for 25 small (H r > 5) dynamically excited trans-Neptunian objects (TNOs) and centaurs acquired as part of the Colours of the Outer Solar System Origins…

2019 The Astronomical Journal
eHST 35
OGLE-2018-BLG-1011Lb,c: Microlensing Planetary System with Two Giant Planets Orbiting a Low-mass Star
DOI: 10.3847/1538-3881/ab2f74 Bibcode: 2019AJ....158..114H

Stassun, Keivan G.; Han, Cheongho; Udalski, Andrzej +79 more

We report a multiplanetary system found from the analysis of microlensing event OGLE-2018-BLG-1011, for which the light curve exhibits a double-bump anomaly around the peak. We find that the anomaly cannot be fully explained by the binary-lens or binary-source interpretations and its description requires the introduction of an additional lens comp…

2019 The Astronomical Journal
Gaia 35