Search Publications

Discovery of Tidal Tails around the Old Open Cluster NGC 2506
DOI: 10.3847/1538-4357/ab8560 Bibcode: 2020ApJ...894...48G

Gao, Xinhua

We report the discovery of tidal tails around the old open cluster NGC 2506 based on Gaia-DR2. A principal-component analysis and Gaussian mixture model are used to identify extra-tidal stars. We identify 2301 stars closely related to the cluster, 147 of which are likely extra-tidal stars. We find clear evidence for the existence of two well-defin…

2020 The Astrophysical Journal
Gaia 13
When the disc's away, the stars will play: dynamical masses in the nova-like variable KR Aur with a pinch of accretion
DOI: 10.1093/mnras/staa612 Bibcode: 2020MNRAS.494..425R

Gänsicke, B. T.; Koester, D.; Toloza, O. +8 more

We obtained time-resolved optical photometry and spectroscopy of the nova-like variable KR Aurigae in the low state. The spectrum reveals a DAB white dwarf (WD) and a mid-M dwarf companion. Using the companion star's i-band ellipsoidal modulation we refine the binary orbital period to be P = 3.906519 ± 0.000001 h. The light curve and the spectra s…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 13
Eclipsing Binaries in the Open Cluster Ruprecht 147. III. The Triple System EPIC 219552514 at the Main-sequence Turnoff
DOI: 10.3847/1538-4357/ab911b Bibcode: 2020ApJ...896..162T

Torres, Guillermo; Vanderburg, Andrew; Rizzuto, Aaron C. +3 more

Spectroscopic observations are reported for the 2.75 day, double-lined, detached eclipsing binary EPIC 219552514 located at the turnoff of the old nearby open cluster Ruprecht 147. A joint analysis of our radial-velocity measurements and the K2 light curve leads to masses of ${M}_{1}={1.509}_{-0.056}^{+0.063}\,{M}_{\odot }$ and ${M}_{2}={0.649}_{-…

2020 The Astrophysical Journal
Gaia 13
Water megamaser emission in hard X-ray selected AGN
DOI: 10.1051/0004-6361/201937407 Bibcode: 2020A&A...641A.162P

Ubertini, P.; Malizia, A.; Bassani, L. +4 more

Context. Water megamaser emission at 22 GHz has proven to be a powerful tool for astrophysical studies of active galactic nuclei (AGN) because it allows an accurate determination of the mass of the central black hole and of the accretion disc geometry and dynamics. However, after searches among thousands of galaxies, only about 200 of them have sh…

2020 Astronomy and Astrophysics
INTEGRAL 13
OGLE-ing the Magellanic System: Cepheids in the Bridge
DOI: 10.3847/1538-4357/ab61f1 Bibcode: 2020ApJ...889...25J

Udalski, Andrzej; Mróz, Przemek; Szymański, Michał K. +12 more

We present a detailed analysis of the Magellanic Bridge Cepheid sample constructed using the Optical Gravitational Lensing Experiment Collection of Variable Stars. Our updated Bridge sample contains 10 classical and 13 anomalous Cepheids. We calculate their individual distances using optical period-Wesenheit relations and construct three-dimension…

2020 The Astrophysical Journal
Gaia 13
Measuring the Heating and Cooling of the Interstellar Medium at High Redshift: PAH and [C II] Observations of the Same Star-forming Galaxies at z ∼ 2
DOI: 10.3847/1538-4357/ab77b9 Bibcode: 2020ApJ...892..119M

Kirkpatrick, Allison; Dickinson, Mark E.; McKinney, Jed +4 more

Star formation depends critically on cooling mechanisms in the interstellar medium (ISM); however, thermal properties of gas in galaxies at the peak epoch of star formation (z ∼ 2) remain poorly understood. A limiting factor in understanding the multiphase ISM is the lack of multiple tracers detected in the same galaxies, such as Polycyclic Aromat…

2020 The Astrophysical Journal
Herschel eHST 13
On the Absence of High-redshift AGNs: Little Growth in the Supermassive Black Hole Population at High Redshifts
DOI: 10.3847/1538-4357/ab6aaa Bibcode: 2020ApJ...891...69C

Bauer, F. E.; Barger, A. J.; Cowie, L. L. +1 more

We search for high-redshift (z > 4.5) X-ray active galactic nuclei (AGNs) in the deep central (off-axis angle < 5'7) region of the 7 Ms Chandra Deep Field-South X-ray image. We compile an initial candidate sample from direct X-ray detections. We then probe more deeply in the X-ray data by using preselected samples with high spatial resolutio…

2020 The Astrophysical Journal
eHST 13
HATS-47b, HATS-48Ab, HATS-49b, and HATS-72b: Four Warm Giant Planets Transiting K Dwarfs
DOI: 10.3847/1538-3881/ab7821 Bibcode: 2020AJ....159..173H

Latham, David W.; Jordán, Andrés; Butler, R. P. +43 more

We report the discovery of four transiting giant planets around K dwarfs. The planets HATS-47b, HATS-48Ab, HATS-49b, and HATS-72b have masses of ${0.369}_{-0.021}^{+0.031} ${M}_{{\rm{J}}}, ${0.243}_{-0.030}^{+0.022} ${M}_{{\rm{J}}}, ${0.353}_{-0.027}^{+0.038} ${M}_{{\rm{J}}}, and $0.1254\pm 0.0039 ${M}_{{\rm{J}}}, respectively, and radii of $1.117…

2020 The Astronomical Journal
Gaia 12
Robust diffraction-limited near-infrared-to-near-ultraviolet wide-field imaging from stratospheric balloon-borne platforms—Super-pressure Balloon-borne Imaging Telescope performance
DOI: 10.1063/1.5139711 Bibcode: 2020RScI...91c4501R

Jauzac, Mathilde; Tam, Sut-Ieng; Benton, Steven J. +26 more

At a fraction of the total cost of an equivalent orbital mission, scientific balloon-borne platforms, operating above 99.7% of the Earth's atmosphere, offer attractive, competitive, and effective observational capabilities—namely, space-like seeing, transmission, and backgrounds—which are well suited for modern astronomy and cosmology. The Super-p…

2020 Review of Scientific Instruments
Gaia 12
A Magnetic White Dwarf Accretion Model for the Anomalous X-Ray Pulsar 4U 0142+61
DOI: 10.3847/1538-4357/ab8add Bibcode: 2020ApJ...895...26B

Rodrigues, Claudia V.; Coelho, Jaziel G.; Castro, Manuel +2 more

The quiescent emission of the anomalous X-ray pulsar (AXP) 4U 0142+61 extends over a broad range of energy, from radio up to hard X-rays. In particular, this object is unique among soft gamma-ray repeaters (SGRs) and AXPs in presenting simultaneously mid-infrared emission and pulsed optical emission. In spite of the many propositions to explain th…

2020 The Astrophysical Journal
INTEGRAL 12