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Single-lined Spectroscopic Binary Star Candidates from a Combination of the RAVE and Gaia DR2 Surveys
DOI: 10.3847/1538-3881/ab3cc1 Bibcode: 2019AJ....158..155B

Grebel, Eva K.; Steinmetz, Matthias; Bland-Hawthorn, Joss +11 more

The combination of the final version of the Radial Velocity Experiment (RAVE) spectroscopic survey data release 6 with radial velocities (RVs) and astrometry from Gaia DR2 allows us to identify and create a catalog of single-lined binary star candidates (SB1), their inferred orbital parameters, and to inspect possible double-lined binary stars (SB…

2019 The Astronomical Journal
Gaia 18
Understanding Formation of Young, Distributed Low-mass Stars and Clusters in the W4 Cloud Complex
DOI: 10.3847/1538-3881/aafbe6 Bibcode: 2019AJ....157..112P

Samal, Manash R.; Sharma, Saurabh; Panwar, Neelam +2 more

It is well known that most of the stars form in rich clusters. However, recent Spitzer observations have shown that a significant number of stars also form in the distributed mode; their origin is not well understood. In this work, we aim to investigate clustered and distributed modes of star formation in the W4 complex. To do so, we identified an…

2019 The Astronomical Journal
Gaia 17
Hubble Ultraviolet Spectroscopy of Jupiter Trojans
DOI: 10.3847/1538-3881/ab0e00 Bibcode: 2019AJ....157..161W

Ehlmann, Bethany L.; Brown, Michael E.; Mahjoub, Ahmed +2 more

We present the first ultraviolet spectra of Jupiter Trojans. These observations were carried out using the Space Telescope Imaging Spectrograph on the Hubble Space Telescope and cover the wavelength range 200-550 nm at low resolution. The targets include objects from both of the Trojan color subpopulations (less-red and red). We do not observe any…

2019 The Astronomical Journal
eHST 17
K2-287 b: An Eccentric Warm Saturn Transiting a G-dwarf
DOI: 10.3847/1538-3881/aafa79 Bibcode: 2019AJ....157..100J

Henning, Thomas; Jordán, Andrés; Espinoza, Néstor +23 more

We report the discovery of K2-287b, a Saturn mass planet orbiting a G-dwarf with a period of P ≈ 15 days. First uncovered as a candidate using K2 campaign 15 data, follow-up photometry and spectroscopy were used to determine a mass {M}{{P}}=0.317+/- 0.026 {M}{{J}}, radius {R}{{P}}=0.833+/- 0.013 {R}{{J}}…

2019 The Astronomical Journal
Gaia 17
Physical Properties of the Close-in Tertiary in the Southern Triple-lined System VZ Lib
DOI: 10.3847/1538-3881/ab17d4 Bibcode: 2019AJ....157..207L

Qian, S. -B.; Liao, W. -P.; Sarotsakulchai, T.

VZ Lib is a southern triple-lined system. By analyzing all available times of light minima, orbital period changes are revisited in detail. We discovered that the observed-calculated (O - C) curve shows a long-term period decrease at a rate of {dP}/{dt}=-2.25× {10}-7 {days yr}}-1, revealing a mass transfer from the more massi…

2019 The Astronomical Journal
Gaia 17
The Blueshift of the C IV Broad Emission Line in QSOs
DOI: 10.3847/1538-3881/ab0956 Bibcode: 2019AJ....157..148G

Bian, Wei-Hao; Ge, Xue; Zhao, Bi-Xuan +1 more

For the sample from Ge et al. of 87 low-z Palomar-Green quasi-stellar objects (QSOs) and 130 high-z QSOs (0 < z < 5) with {{H}}β -based single-epoch supermassive black hole masses, we perform a uniform decomposition of the C IV λ1549 broad-line profile. Based on the rest frame defined by the [O III] λ5007 narrow emission line, a medium-stron…

2019 The Astronomical Journal
IUE eHST 17
Spectroscopic Mass and Host-star Metallicity Measurements for Newly Discovered Microlensing Planet OGLE-2018-BLG-0740Lb
DOI: 10.3847/1538-3881/ab2df4 Bibcode: 2019AJ....158..102H

Kollmeier, Juna A.; Morrell, Nidia; Han, Cheongho +67 more

We report the discovery of the microlensing planet OGLE-2018-BLG-0740Lb. The planet is detected with a very strong signal of Δχ 2 ∼ 4630, but the interpretation of the signal suffers from two types of degeneracies. One type is caused by the previously known close/wide degeneracy, and the other is caused by an ambiguity between two solut…

2019 The Astronomical Journal
Gaia 17
Resolved Imaging of the AR Puppis Circumbinary Disk
DOI: 10.3847/1538-3881/aafe04 Bibcode: 2019AJ....157..110E

Marshall, J. P.; Ertel, S.; Milli, J. +14 more

Circumbinary disks are common around post-asymptotic giant branch (post-AGB) stars with a stellar companion on orbital timescales of a few 100 to few 1000 days. The presence of a disk is usually inferred from the system’s spectral energy distribution and confirmed, for a sub-sample, by interferometric observations. We used the Spectro-Polarimetric…

2019 The Astronomical Journal
AKARI 16
K2-288Bb: A Small Temperate Planet in a Low-mass Binary System Discovered by Citizen Scientists
DOI: 10.3847/1538-3881/aafa70 Bibcode: 2019AJ....157...40F

Schlieder, Joshua E.; Howard, Andrew W.; Petigura, Erik A. +23 more

Observations from the Kepler and K2 missions have provided the astronomical community with unprecedented amounts of data to search for transiting exoplanets and other astrophysical phenomena. Here, we present K2-288, a low-mass binary system (M2.0 ± 1.0; M3.0 ± 1.0) hosting a small (R p = 1.9 R ), temperate (T eq

2019 The Astronomical Journal
Gaia 16
Visual Orbits of Spectroscopic Binaries with the CHARA Array. I. HD 224355
DOI: 10.3847/1538-3881/ab064d Bibcode: 2019AJ....157..140L

Gies, Douglas R.; Lester, Kathryn V.; Monnier, John D. +5 more

We present the visual orbit of the double-lined spectroscopic binary HD 224355 from interferometric observations with the CHARA Array, as well as an updated spectroscopic analysis using echelle spectra from the Apache Point Observatory 3.5 m telescope. By combining the visual and spectroscopic orbital solutions, we find the binary components to ha…

2019 The Astronomical Journal
Gaia 16