Search Publications

Nearby Quintuple Systems κ Tucanae and ξ Scorpii
DOI: 10.3847/1538-3881/ab8af1 Bibcode: 2020AJ....159..265T

Tokovinin, Andrei

Architecture and parameters of two wide, nearby hierarchical systems containing five solar-type stars each, κ Tuc and ξ Sco, are studied. Using Gaia astrometry and photometry, masses are determined from visual orbits and isochrones, and effective temperatures from spectra or colors. Both systems are ∼2 Gyr old. Their spatial motion corresponds to …

2020 The Astronomical Journal
Gaia 5
Identifying Exo-Earth Candidates in Direct Imaging Data through Bayesian Classification
DOI: 10.3847/1538-3881/ab5222 Bibcode: 2020AJ....159....3B

Apai, Dániel; Bixel, Alex

Future space telescopes may be able to directly image between approximately 10 and 100 planets with sizes and orbits consistent with habitable surface conditions (“exo-Earth candidates” or EECs), but observers will face difficulty in distinguishing these from the potentially hundreds of nonhabitable “false positives” which will also be detected. T…

2020 The Astronomical Journal
Gaia 5
The Statistics of Extended Debris Disks Measured with Gaia and Planck
DOI: 10.3847/1538-3881/ab8192 Bibcode: 2020AJ....159..210N

Jain, Bhuvnesh; Nibauer, Jacob; Baxter, Eric

Thermal emission from debris disks around stars has been measured using targeted and resolved observations. We present an alternative likelihood-based approach in which temperature maps from the Planck cosmic microwave background (CMB) survey at 857 and 545 GHz are analyzed in conjunction with stellar positions from Gaia to estimate the fraction o…

2020 The Astronomical Journal
Gaia 5
Searching the Entirety of Kepler Data. I. 17 New Planet Candidates Including One Habitable Zone World
DOI: 10.3847/1538-3881/ab6cf8 Bibcode: 2020AJ....159..124K

Kunimoto, Michelle; Ngo, Henry; Matthews, Jaymie M.

We present the results of an independent search of all ∼200,000 stars observed over the four year Kepler mission (Q1-Q17) for multiplanet systems, using a three-transit minimum detection criterion to search orbital periods up to hundreds of days. We incorporate both automated and manual triage, and provide estimates of the completeness and reliabi…

2020 The Astronomical Journal
Gaia 5
Spatially Resolved Velocity Structures in Jets of DF Tau and UY Aur A
DOI: 10.3847/1538-3881/ab91a3 Bibcode: 2020AJ....160...39U

Principe, David A.; Günther, Hans Moritz; Schneider, P. Christian +1 more

Young stars accrete mass and angular momentum from their circumstellar disks. Some of them also drive outflows, which can be distinguished in optical forbidden emission lines. We analyze a sample of binary T Tauri stars observed with long-slit spectroscopy by the Hubble Space Telescope between 1998 and 2000, searching for spatially resolved outflo…

2020 The Astronomical Journal
Gaia eHST 4
X-Ray Observations of the Peculiar Cepheid V473 Lyr Identify A Low-mass Companion
DOI: 10.3847/1538-3881/ab7121 Bibcode: 2020AJ....159..121E

Drake, Jeremy J.; Evans, Nancy Remage; Marengo, Massimo +17 more

V473 Lyr is a classical Cepheid that is unique in having substantial amplitude variations with a period of approximately 3.3 yr, thought to be similar to the Blazhko variations in RR Lyrae stars. We obtained an XMM-Newton observation of this star to follow up a previous detection in X-rays. Rather than the X-ray burst and rapid decline near maximu…

2020 The Astronomical Journal
Gaia XMM-Newton eHST 4
A Spectroscopic Classification Survey to Search for New ρ Puppis Stars
DOI: 10.3847/1538-3881/ab974c Bibcode: 2020AJ....160...52M

Gray, Richard O.; McGahee, Courtney; Griffin, R. E. M. +2 more

The ρ Puppis stars are mid-F-type stars that show peculiar chemical-abundance patterns similar to those of the Am stars. Typically they exhibit overabundances of iron-peak elements such as Fe and Ni and s- and r-process elements such as Sr and Eu, and underabundances of certain other elements including He, Ca, and Sc. It has been proposed that the…

2020 The Astronomical Journal
Gaia 4
The Quadruple System HIP 45734
DOI: 10.3847/1538-3881/ab6a13 Bibcode: 2020AJ....159...88T

Tokovinin, Andrei

HIP 45734 is a quadruple system of 2 + 2 architecture located at 68 pc from the Sun. The outer 9″ system A,B has a period of ∼104 yr. The subsystem Aa,Ab is a visual binary with a period of 20.1 yr and an eccentricity of 0.78. Its periastron in 2019.1 was observed spectroscopically, yielding masses (1.10 ± 0.04 and 0.98 ± 0.03 ${{ \math…

2020 The Astronomical Journal
Gaia 4
Estimating the Ages of FGK Dwarf Stars through the Use of GALEX FUV Magnitudes
DOI: 10.3847/1538-3881/abb77d Bibcode: 2020AJ....160..217C

Crandall, Sara; Smith, Graeme H.; Subramonian, Arjun +2 more

Stellar age cannot be directly measured, yet age determinations are fundamental to understanding the evolution of stars, planets, and galaxies. The work presented here builds upon the idea of a stellar-activity age. We utilized far-ultraviolet (FUV) photometry acquired by the Galaxy Evolution Explorer (GALEX) space telescope as an indicator of chr…

2020 The Astronomical Journal
IUE 4
Optical Studies of Eight AM Herculis-type Cataclysmic Variable Stars
DOI: 10.3847/1538-3881/ab9d1b Bibcode: 2020AJ....160...70T

Thorstensen, John R.; Buckley, David A. H.; Woudt, Patrick A. +2 more

We report detailed follow-up observations of eight cataclysmic variable stars (CVs) that are apparently AM Her stars, also called polars. For all, we either determine orbital periods for the first time or improve on existing determinations. The seven for which we have spectra show the high-amplitude radial-velocity curves and prominent He II λ4686…

2020 The Astronomical Journal
Gaia 4