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Census of the Young Stellar Population in the Galactic H II Region Sh2-242
DOI: 10.3847/1538-3881/ab737a Bibcode: 2020AJ....159..153P

Joshi, Santosh; Dutta, Somnath; Mondal, Soumen +3 more

We present here identification and characterization of the young stellar population associated with an active star-forming site Sh2-242. We used our own new optical imaging and spectroscopic observational data, as well as several archival catalogs, e.g., Pan-STARRS 1, Gaia DR2, IPHAS, Wide-field InfraRed Camera, 2MASS, and Spitzer. Slit spectrosco…

2020 The Astronomical Journal
Gaia 3
Orbital Refinement and Stellar Properties for the HD 9446, HD 43691, and HD 179079 Planetary Systems
DOI: 10.3847/1538-3881/ab7d33 Bibcode: 2020AJ....159..197H

Henry, Gregory W.; Kane, Stephen R.; Pepper, Joshua +15 more

The Transit Ephemeris Refinement and Monitoring Survey is a project that aims to detect transits of intermediate-long period planets by refining orbital parameters of the known radial velocity planets using additional data from ground-based telescopes, calculating a revised transit ephemeris for the planet, then monitoring the planet host star dur…

2020 The Astronomical Journal
Gaia 2
Open Cluster IC 1369 and Its Vicinity: Multicolor Photometry and Gaia DR2 Astrometry
DOI: 10.3847/1538-3881/ab67b5 Bibcode: 2020AJ....159...95S

Straižys, V.; Raudeliūnas, S.; Maskoliūnas, M. +9 more

The open cluster IC 1369, located in Cygnus close to the galactic equator at the 89°6 longitude, and its vicinity are investigated by applying two-dimensional photometric classification of stars down to V = 19 mag measured in the Vilnius seven-color photometric system. Employing the Gaia DR2 coordinates, parallaxes, and proper motions, 143 cluster…

2020 The Astronomical Journal
Gaia 2
Emission-line Data Cubes of the HH 32 Stellar Jet
DOI: 10.3847/1538-3881/abadfa Bibcode: 2020AJ....160..165H

Hartigan, Patrick; Neill, James D.; Hillenbrand, Lynne A. +5 more

We analyze data cubes of over 60 emission lines in the HH 32 stellar jet acquired with the Keck Cosmic Web Imager (KCWI). The data cover the less explored blue portion of the spectrum between 3586 and 6351 Å and have both high spectral (R ∼ 10,000) and spatial (≲1″) resolution. The study includes all three major ionization states of oxygen, three …

2020 The Astronomical Journal
Gaia eHST 2
A KELT-TESS Eclipsing Binary in a Young Triple System Associated with the Local "Stellar String" Theia 301
DOI: 10.3847/1538-3881/abafaf Bibcode: 2020AJ....160..187C

Cunningham, Joni-Marie C.; Feliz, Dax L.; Dixon, Don M. +10 more

HD 54236 is a nearby, wide common-proper-motion visual pair that has been previously identified as likely being very young by virtue of strong X-ray emission and lithium absorption. Here, we report the discovery that the brighter member of the wide pair, HD 54236A, is itself an eclipsing binary (EB), comprising two near-equal solar-mass stars on a…

2020 The Astronomical Journal
Gaia 2
HD 165054: An Astrometric Calibration Field for High-contrast Imagers in Baade's Window
DOI: 10.3847/1538-3881/ab86aa Bibcode: 2020AJ....159..244N

Duchêne, Gaspard; Esposito, Thomas M.; Hom, Justin +51 more

We present a study of the HD 165054 astrometric calibration field that has been periodically observed with the Gemini Planet Imager (GPI). HD 165054 is a bright star within Baade's Window, a region of the galactic plane with relatively low extinction from interstellar dust. HD 165054 was selected as a calibrator target due to the high number densi…

2020 The Astronomical Journal
Gaia 2
Chandra Resolves the Double FU Orionis System RNO 1B/1C in X-Rays
DOI: 10.3847/1538-3881/ab846b Bibcode: 2020AJ....159..221S

Skinner, Stephen L.; Güdel, Manuel

We present new Chandra X-ray observations of the close pair of young stars RNO 1B and 1C (6″ separation) located in the L1287 cloud. RNO 1B erupted in 1978-1990 and is classified as an FU Orionis star (FUor). RNO 1C also shows most of the properties of an FUor but no eruption has been seen yet. Only a few dozen FUors are known and the presence of …

2020 The Astronomical Journal
Gaia XMM-Newton 2
Exoplanets in the Antarctic Sky. IV. Dual-band Photometry of Variables Found by the CSTAR-II Commissioning Survey at the North Sky
DOI: 10.3847/1538-3881/ab7449 Bibcode: 2020AJ....159..172Z

Wittenmyer, Robert A.; Wang, Lifan; Yang, Ming +30 more

From the experiences learned in three decades of exoplanet search, wide-field transit surveys have proven to be one of the most effective ways to detect exoplanets. Wide field of view, however, suffers from high false-positive rates caused by blended eclipsing binaries. The chromaticity in eclipse depth is an effective feature to distinguish low-d…

2020 The Astronomical Journal
Gaia 2
Massive Stars in Molecular Clouds Rich in High-energy Sources: The Bridge of G332.809-0.132 and CS 78 in NGC 6334
DOI: 10.3847/1538-3881/ab9950 Bibcode: 2020AJ....160...65M

Menten, Karl M.; Figer, Donald F.; Messineo, Maria +1 more

Detections of massive stars in the direction of the H II region CS 78 in NGC 6334 and of G332.809-0.132 are here presented. The region covered by the G332.809-0.132 complex coincides with the RCW 103 stellar association. In its core (40' in radius), approximately 110 OB candidate stars (Ks < 10 mag and 0.4 < ${A}_{{K}_{s}}$ < 1…

2020 The Astronomical Journal
Gaia 1
Detecting Exoplanets Using Eclipsing Binaries as Natural Starshades
DOI: 10.3847/1538-3881/aba7c6 Bibcode: 2020AJ....160..131B

Zabludoff, Ann I.; Guyon, Olivier; Bellotti, Stefano +2 more

We investigate directly imaging exoplanets around eclipsing binaries using the eclipse as a natural tool for dimming the binary and thus increasing the planet to star brightness contrast. At eclipse, the binary becomes pointlike, making coronagraphy possible. We select binaries where the planet-star contrast would be boosted by >10× during ecli…

2020 The Astronomical Journal
Gaia 1