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Empirical Bolometric Fluxes and Angular Diameters of 1.6 Million Tycho-2 Stars and Radii of 350,000 Stars with Gaia DR1 Parallaxes
DOI: 10.3847/1538-3881/aa957b Bibcode: 2017AJ....154..259S

Stassun, Keivan G.; Stevens, Daniel J.; Gaudi, B. Scott

We present bolometric fluxes and angular diameters for over 1.6 million stars in the Tycho-2 catalog, determined using previously determined empirical color-temperature and color-flux relations. We vet these relations via full fits to the full broadband spectral energy distributions for a subset of benchmark stars and perform quality checks agains…

2017 The Astronomical Journal
Gaia Hipparcos 36
Detection of a Hydrogen Corona in HST Lyα Images of Europa in Transit of Jupiter
DOI: 10.3847/1538-3881/153/2/67 Bibcode: 2017AJ....153...67R

Roth, Lorenz; Strobel, Darrell F.; Becker, Tracy M. +4 more

We report far-ultraviolet observations of Europa in transit of Jupiter obtained with the Space Telescope Imaging Spectrograph of the Hubble Space Telescope on six occasions between 2014 December and 2015 March. Absorption of Jupiter’s bright hydrogen Lyα dayglow is detected in a region several moon radii above the limb in all observations. The obs…

2017 The Astronomical Journal
eHST 36
Gaia Assorted Mass Binaries Long Excluded from SLoWPoKES (GAMBLES): Identifying Ultra-wide Binary Pairs with Components of Diverse Mass
DOI: 10.3847/1538-3881/aa6d55 Bibcode: 2017AJ....153..259O

Stassun, Keivan G.; Oelkers, Ryan J.; Dhital, Saurav

The formation and evolution of binary star systems are some of the remaining key questions in modern astronomy. Wide binary pairs (separations >103 au) are particularly intriguing because their low binding energies make it difficult for the stars to stay gravitationally bound over extended timescales, and thus to probe the dynamics o…

2017 The Astronomical Journal
Gaia 35
The Star Blended with the MOA-2008-BLG-310 Source Is Not the Exoplanet Host Star
DOI: 10.3847/1538-3881/aa7b80 Bibcode: 2017AJ....154...59B

Bennett, D. P.; Anderson, J.; Gould, A. +7 more

High-resolution Hubble Space Telescope (HST) image analysis of the MOA-2008-BLG-310 microlens system indicates that the excess flux at the location of the source found in the discovery paper cannot primarily be due to the lens star because it does not match the lens-source relative proper motion, {µ }{rel}, predicted by the microl…

2017 The Astronomical Journal
eHST 35
Characterization of the VVV Survey RR Lyrae Population across the Southern Galactic Plane
DOI: 10.3847/1538-3881/aa5be4 Bibcode: 2017AJ....153..179M

Valenti, Elena; Minniti, Dante; Rejkuba, Marina +14 more

Deep near-IR images from the VISTA Variables in the Vía Láctea (VVV) Survey were used to search for RR Lyrae stars in the Southern Galactic plane. A sizable sample of 404 RR Lyrae of type ab stars was identified across a thin slice of the fourth Galactic quadrant (295° < ℓ < 350°, -2.°24 < b < -1.°05). The sample’s distance distributio…

2017 The Astronomical Journal
Gaia 35
The Structure of Chariklo’s Rings from Stellar Occultations
DOI: 10.3847/1538-3881/aa830d Bibcode: 2017AJ....154..144B

Colas, F.; Bérard, D.; Kervella, P. +79 more

Two narrow and dense rings (called C1R and C2R) were discovered around the Centaur object (10199) Chariklo during a stellar occultation observed on 2013 June 3. Following this discovery, we planned observations of several occultations by Chariklo’s system in order to better characterize the physical properties of the ring and main body. Here, we u…

2017 The Astronomical Journal
Gaia 35
High-resolution Spectroscopy of Extremely Metal-poor Stars from SDSS/SEGUE. III. Unevolved Stars with [Fe/H] ≲ -3.5
DOI: 10.3847/1538-3881/aa7a08 Bibcode: 2017AJ....154...52M

Honda, Satoshi; Beers, Timothy C.; Lee, Young Sun +2 more

We present elemental abundances for eight unevolved extremely metal-poor (EMP) stars with {T}{eff}> 5500 {{K}}, among which seven have [{Fe}/{{H}}]< -3.5. The sample is selected from the Sloan Digital Sky Survey/Sloan Extension for Galactic Understanding and Exploration (SDSS/SEGUE) and our previous high-resolution spectroscopic f…

2017 The Astronomical Journal
Gaia 33
CCD Parallaxes for 309 Late-type Dwarfs and Subdwarfs
DOI: 10.3847/1538-3881/aa880b Bibcode: 2017AJ....154..147D

Harris, Hugh C.; Vrba, Frederick J.; Munn, Jeffrey A. +16 more

New, updated, and/or revised CCD parallaxes determined with the Strand Astrometric Reflector at the Naval Observatory Flagstaff Station are presented. Included are results for 309 late-type dwarf and subdwarf stars observed over the 30+ years that the program operated. For 124 of the stars, parallax determinations from other investigators have alr…

2017 The Astronomical Journal
Gaia 31
The Discovery of λ Bootis Stars: The Southern Survey I
DOI: 10.3847/1538-3881/aa6d5e Bibcode: 2017AJ....154...31G

Neff, J. E.; Cheng, K. -P.; Gray, R. O. +5 more

The λ Boo stars are a class of chemically peculiar Population I A-type stars characterized by under-abundances of the refractory elements, but near-solar abundances of carbon, nitrogen, oxygen, and sulfur. There is some evidence that λ Boo stars have higher frequencies of “bright” debris disks than normal A-type stars. The discovery of four exopla…

2017 The Astronomical Journal
Gaia 31
The Young Substellar Companion ROXs 12 B: Near-infrared Spectrum, System Architecture, and Spin-Orbit Misalignment
DOI: 10.3847/1538-3881/aa88bd Bibcode: 2017AJ....154..165B

Vanderburg, Andrew; Brogi, Matteo; Knutson, Heather A. +8 more

ROXs 12 (2MASS J16262803-2526477) is a young star hosting a directly imaged companion near the deuterium-burning limit. We present a suite of spectroscopic, imaging, and time-series observations to characterize the physical and environmental properties of this system. Moderate-resolution near-infrared spectroscopy of ROXs 12 B from Gemini-North/NI…

2017 The Astronomical Journal
Gaia 31