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The White Dwarf Binary Pathways Survey. V. The Gaia White Dwarf Plus AFGK Binary Sample and the Identification of 23 Close Binaries
DOI: 10.3847/1538-4357/abc017 Bibcode: 2020ApJ...905...38R

Gänsicke, B. T.; Rebassa-Mansergas, A.; Raddi, R. +22 more

Close white dwarf binaries consisting of a white dwarf and an A-, F-, G-, or K-type main-sequence star, henceforth close WD+AFGK binaries, are ideal systems to understand the nature of type Ia supernovae progenitors and to test binary evolution models. In this work we identify 775 WD+AFGK candidates from TGAS (The Tycho-Gaia Astrometric Solution) …

2020 The Astrophysical Journal
Gaia 25
The Vanishing and Appearing Sources during a Century of Observations Project. I. USNO Objects Missing in Modern Sky Surveys and Follow-up Observations of a “Missing Star”
DOI: 10.3847/1538-3881/ab570f Bibcode: 2020AJ....159....8V

Gupta, Alok C.; Kochukhov, Oleg; Krisciunas, Kevin +19 more

In this paper we report the current status of a new research program. The primary goal of the “Vanishing and Appearing Sources during a Century of Observations” project is to search for vanishing and appearing sources using existing survey data to find examples of exceptional astrophysical transients. The implications of finding such objects exten…

2020 The Astronomical Journal
Gaia 25
Discovery of a Remarkably Powerful Broad Absorption-line Quasar Outflow in SDSS J135246.37+423923.5
DOI: 10.3847/1538-4357/ab6f72 Bibcode: 2020ApJ...891...53C

Gallagher, Sarah C.; Terndrup, Donald M.; Leighly, Karen M. +2 more

Broad absorption-line (BAL) features in quasar spectra reveal an unambiguous signature of energetic outflows from central supermassive black holes, and thus, BAL quasars are prime targets for investigating the potential process of luminous quasar feedback on galaxies. We analyzed the rest-UV spectrum of an "overlapping trough" iron low-ionization …

2020 The Astrophysical Journal
Herschel eHST 25
The Formation Height of Millimeter-wavelength Emission in the Solar Chromosphere
DOI: 10.3847/2041-8213/ab75ac Bibcode: 2020ApJ...891L...8M

Martínez-Sykora, Juan; De Pontieu, Bart; Chintzoglou, Georgios +1 more

In the past few years, the ALMA radio telescope has become available for solar observations. ALMA diagnostics of the solar atmosphere are of high interest because of the theoretically expected linear relationship between the brightness temperature at millimeter wavelengths and the local gas temperature in the solar atmosphere. Key for the interpre…

2020 The Astrophysical Journal
IRIS 25
The PIPER Survey. I. An Initial Look at the Intergalactic Globular Cluster Population in the Perseus Cluster
DOI: 10.3847/1538-4357/ab6992 Bibcode: 2020ApJ...890..105H

Wittmann, Carolin; Lisker, Thorsten; Romanowsky, Aaron J. +7 more

We describe the goals and first results of the Program for Imaging of the PERseus cluster of galaxies (PIPER). The first phase of the program builds on imaging of fields obtained with the Hubble Space Telescope (HST) Advanced Camera for Surveys (ACS)/WFC and WFC3/UVIS cameras. Our PIPER target fields with HST include major early-type galaxies incl…

2020 The Astrophysical Journal
eHST 25
The Pan-Pacific Planet Search - VIII. Complete results and the occurrence rate of planets around low-luminosity giants
DOI: 10.1093/mnras/stz3378 Bibcode: 2020MNRAS.491.5248W

Butler, R. P.; Wittenmyer, Robert A.; Horner, Jonathan +6 more

Our knowledge of the populations and occurrence rates of planets orbiting evolved intermediate-mass stars lags behind that for solar-type stars by at least a decade. Some radial velocity surveys have targeted these low-luminosity giant stars, providing some insights into the properties of their planetary systems. Here, we present the final data re…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 25
Variations in the Ionospheric Peak Altitude at Mars in Response to Dust Storms: 13 Years of Observations From the Mars Express Radar Sounder
DOI: 10.1029/2019JE006092 Bibcode: 2020JGRE..12506092G

Gurnett, D. A.; Němec, F.; Morgan, D. D. +7 more

Previous observations have shown that, during Martian dust storms, the peak of the ionosphere rises in altitude. Observational studies of this type, however, have been extremely limited. Using 13 years of ionospheric peak altitude data from the Mars Advanced Radar for Subsurface and Ionosphere Sounding instrument on Mars Express, we study how the …

2020 Journal of Geophysical Research (Planets)
MEx 25
WISEA J083011.95+283716.0: A Missing Link Planetary-mass Object
DOI: 10.3847/1538-4357/ab8d25 Bibcode: 2020ApJ...895..145B

Wisniewski, John; Kirkpatrick, J. Davy; Burgasser, Adam J. +17 more

We present the discovery of WISEA J083011.95+283716.0, the first Y-dwarf candidate identified through the "Backyard Worlds: Planet 9" citizen science project. We identified this object as a red, fast-moving source with a faint W2 detection in multiepoch AllWISE and unWISE images. We have characterized this object with Spitzer and Hubble Space Tele…

2020 The Astrophysical Journal
eHST 25
Searching for proto-planets with MUSE
DOI: 10.1051/0004-6361/202038242 Bibcode: 2020A&A...644A.149X

Snellen, I. A. G.; Girard, J.; Brinchmann, J. +5 more

Context. Protoplanetary disks contain structures such as gaps, rings, and spirals, which are thought to be produced by the interaction between the disk and embedded protoplanets. However, only a few planet candidates are found orbiting within protoplanetary disks, and most of them are being challenged as having been confused with disk features.

2020 Astronomy and Astrophysics
Gaia 25
ALMA CO Observations of Gamma-Ray Supernova Remnant N132D in the Large Magellanic Cloud: Possible Evidence for Shocked Molecular Clouds Illuminated by Cosmic-Ray Protons
DOI: 10.3847/1538-4357/abb469 Bibcode: 2020ApJ...902...53S

Filipović, M. D.; Vink, J.; Rowell, G. +23 more

N132D is the brightest gamma-ray supernova remnant (SNR) in the Large Magellanic Cloud (LMC). We carried out 12CO(J = 1-0, 3-2) observations toward the SNR using the Atacama Large Millimeter/submillimeter Array (ALMA) and Atacama Submillimeter Telescope Experiment. We find diffuse CO emission not only at the southern edge of the SNR as …

2020 The Astrophysical Journal
eHST 25