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Dippers from the TESS Full-frame Images. I. Results of the First One Year Data and Discovery of a Runaway Dipper
DOI: 10.3847/1538-4365/abbc17 Bibcode: 2020ApJS..251...18T

Takita, Satoshi; Hattori, Kohei; Muto, Takayuki +9 more

We present a comprehensive catalog of the dippers—young stellar objects that exhibit episodic dimming—derived from one year's worth of data of the Transiting Exoplanet Survey Satellite (TESS) full-frame images. In the survey, we found 35 dippers using the convolutional neural network, most of them newly discovered. Although these dippers are widel…

2020 The Astrophysical Journal Supplement Series
AKARI Gaia 20
VERITAS Discovery of VHE Emission from the Radio Galaxy 3C 264: A Multiwavelength Study
DOI: 10.3847/1538-4357/ab910e Bibcode: 2020ApJ...896...41A

Fortin, P.; Archer, A.; Benbow, W. +67 more

The radio source 3C 264, hosted by the giant elliptical galaxy NGC 3862, was observed with the Very Energetic Radiation Imaging Telescope Array System (VERITAS) between 2017 February and 2019 May. These deep observations resulted in the discovery of very high energy (VHE; E > 100 GeV) γ-ray emission from this active galaxy. An analysis of ∼57 h…

2020 The Astrophysical Journal
eHST 20
Photometric and kinematic study of the three intermediate age open clusters NGC 381, NGC 2360, and Berkeley 68
DOI: 10.1093/mnras/staa893 Bibcode: 2020MNRAS.494.4713M

Joshi, Y. C.; Maurya, Jayanand

We present UBVRcIc photometric study of three intermediate age open star clusters NGC 381, NGC 2360, and Berkeley 68 (Be 68). We examine the cluster membership of stars using recently released Gaia DR2 proper motions and obtain a total of 116, 332, and 264 member stars in these three clusters. The mean reddening of E(B - V) =…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 20
Multiwavelength Polarimetry of the Filamentary Cloud IC 5146. II. Magnetic Field Structures
DOI: 10.3847/1538-4357/ab5c1c Bibcode: 2020ApJ...888...13W

Wang, Jia-Wei; Lai, Shih-Ping; Eswaraiah, Chakali +4 more

The IC 5146 cloud is a nearby star-forming region in Cygnus, consisting of molecular gas filaments in a variety of evolutionary stages. We used optical and near-infrared polarization data toward the IC 5146 cloud, reported in the first paper of this series, to reveal the magnetic fields in this cloud. Using the newly released Gaia data, we found t…

2020 The Astrophysical Journal
Gaia 20
Expectations on mass determination using astrometric microlensing by Gaia
DOI: 10.1051/0004-6361/201937061 Bibcode: 2020A&A...640A..83K

Bastian, U.; Wambsganss, J.; Klüter, J.

Context. Astrometric gravitational microlensing can be used to determine the mass of a single star (the lens) with an accuracy of a few percent. To do so, precise measurements of the angular separations between lens and background star with an accuracy below 1 milli - arcsec at different epochs are needed. Therefore only the most accurate instrume…

2020 Astronomy and Astrophysics
Gaia 20
Is the gap in the DS Tau disc hiding a planet?
DOI: 10.1093/mnras/staa1278 Bibcode: 2020MNRAS.495.1913V

Herczeg, Gregory J.; Long, Feng; Pinte, Christophe +6 more

Recent millimetre-wavelength surveys performed with the Atacama Large Millimeter Array (ALMA) have revealed protoplanetary discs characterized by rings and gaps. A possible explanation for the origin of such rings is the tidal interaction with an unseen planetary companion. The protoplanetary disc around DS Tau shows a wide gap in the ALMA observa…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 20
Mawrth Vallis, Mars: A Fascinating Place for Future In Situ Exploration
DOI: 10.1089/ast.2019.2074 Bibcode: 2020AsBio..20..199P

Horgan, Briony; Poulet, François; Carter, John +4 more

After the successful landing of the Mars Science Laboratory rover, both NASA and ESA initiated a selection process for potential landing sites for the Mars2020 and ExoMars missions, respectively. Two ellipses located in the Mawrth Vallis region were proposed and evaluated during a series of meetings (three for Mars2020 mission and five for ExoMars…

2020 Astrobiology
MEx 20
A Ringed Pole-on Outflow from DO Tauri Revealed by ALMA
DOI: 10.3847/1538-3881/ab7a10 Bibcode: 2020AJ....159..171F

Zapata, Luis A.; Rodríguez, Luis F.; Guzmán, Andrés E. +3 more

We present new Atacama Large Millimeter/submillimeter Array (ALMA) Band 6 observations including the CO(2-1) line and 1.3 mm continuum emission from the surroundings of the young stellar object DO Tauri. The ALMA CO molecular data show three different series of rings at different radial velocities. These rings have radii around 220 and 800 au. We …

2020 The Astronomical Journal
Gaia eHST 20
Interaction of electron acoustic waves in the presence of superthermal electrons in terrestrial magnetosphere
DOI: 10.1063/1.5143400 Bibcode: 2020PhPl...27d2105J

Masood, W.; Jahangir, R.

We have investigated the propagation and interaction of nonlinear electron acoustic waves (EAWs) in a plasma comprising hot (superthermal) and cold electrons and immobile ions. We have derived the Korteweg-de Vries equation for EAWs in the small amplitude limit. Employing the Hirota's Direct method, we have investigated the multisoliton solutions …

2020 Physics of Plasmas
Cluster 20
Cometary Comae-Surface Links
DOI: 10.1007/s11214-020-00744-0 Bibcode: 2020SSRv..216..130M

Skorov, Yuri; Kappel, David; Vincent, Jean-Baptiste +9 more

A comet is a highly dynamic object, undergoing a permanent state of change. These changes have to be carefully classified and considered according to their intrinsic temporal and spatial scales. The Rosetta mission has, through its contiguous in-situ and remote sensing coverage of comet 67P/Churyumov-Gerasimenko (hereafter 67P) over the time span …

2020 Space Science Reviews
Rosetta 20