Search Publications

The Solar Neighborhood. XLVI. Revealing New M Dwarf Binaries and Their Orbital Architectures
DOI: 10.3847/1538-3881/abb4e9 Bibcode: 2020AJ....160..215V

Henry, Todd J.; Jao, Wei-Chun; Vrijmoet, Eliot Halley +1 more

We use 20 yr of astrometric data from the REsearch Consortium On Nearby Stars (RECONS) program on the Cerro Tololo Inter-American Observatory/SMARTS 0.9 m telescope to provide new insight into multiple star systems in the solar neighborhood. We provide new and updated parallaxes for 210 systems and derive nine high-quality astrometric orbits with …

2020 The Astronomical Journal
Gaia 23
Magnetosheath Jets and Plasmoids: Characteristics and Formation Mechanisms from Hybrid Simulations
DOI: 10.3847/2041-8213/abad2b Bibcode: 2020ApJ...900L...6P

Blanco-Cano, Xóchitl; Burgess, David; Trotta, Domenico +2 more

Magnetosheath jets and plasmoids are very common phenomena downstream of Earth's quasi-parallel bow shock. As the increase of the dynamic pressure is one of the principal characteristics of magnetosheath jets, the embedded paramagnetic plasmoids have been considered as an special case of the former. Although the properties of both types of structu…

2020 The Astrophysical Journal
Cluster 23
SOFIA/FORCAST Galactic Center Legacy Survey: Overview
DOI: 10.3847/1538-4357/ab7c5d Bibcode: 2020ApJ...894...55H

Morris, Mark R.; Longmore, Steven N.; García-Marín, Macarena +12 more

The Galactic Center contains some of the most extreme conditions for star formation in our Galaxy, as well as many other phenomena that are unique to this region. Given our relative proximity to the Galactic Center, we are able to study details of physical processes to a level that is simply not yet possible for more distant galaxies, yielding an …

2020 The Astrophysical Journal
eHST 23
Single magnetic white dwarfs with Balmer emission lines: a small class with consistent physical characteristics as possible signposts for close-in planetary companions
DOI: 10.1093/mnras/staa2969 Bibcode: 2020MNRAS.499.2564G

Gänsicke, Boris T.; Pala, Anna F.; Rodríguez-Gil, Pablo +4 more

We report the identification of SDSS J121929.45+471522.8 as the third apparently isolated magnetic (B ≃ 18.5 ± 1.0 MG) white dwarf exhibiting Zeeman-split Balmer emission lines. The star shows coherent variability at optical wavelengths with an amplitude of ≃0.03 mag and a period of 15.26 h, which we interpret as the spin period of the white dwarf…

2020 Monthly Notices of the Royal Astronomical Society
Gaia 23
Chemistry and Physics of a Low-metallicity Hot Core in the Large Magellanic Cloud
DOI: 10.3847/1538-4357/ab6e6b Bibcode: 2020ApJ...891..164S

Onaka, Takashi; Aikawa, Yuri; Shimonishi, Takashi +5 more

We here present the results of 0.1 pc scale observations in 250 and 350 GHz toward a newly-discovered hot molecular core in a nearby low-metallicity galaxy, the Large Magellanic Cloud (LMC), with the Atacama Large Millimeter/submillimeter Array. A variety of C/N/O/Si/S-bearing molecules are detected toward the high-mass young stellar object, ST16.…

2020 The Astrophysical Journal
AKARI 23
Carbonyl Sulfide (OCS): Detections in Comets C/2002 T7 (LINEAR), C/2015 ER61 (PanSTARRS), and 21P/Giacobini-Zinner and Stringent Upper Limits in 46P/Wirtanen
DOI: 10.3847/1538-3881/aba522 Bibcode: 2020AJ....160..184S

Vervack, Ronald J., Jr.; Kawakita, Hideyo; DiSanti, Michael A. +6 more

Carbonyl sulfide (OCS) is one of the sulfur-bearing molecules detected in different astronomical environments, including comets. The present-day sulfur chemistry in comets may reveal much about the origin of these ices and their subsequent processing history. Cometary sulfur molecules such as H2S, H2CS, SO2, SO, CS…

2020 The Astronomical Journal
Rosetta 23
A census of the nearby Pisces-Eridanus stellar stream. Commonalities with and disparities from the Pleiades
DOI: 10.1051/0004-6361/202037691 Bibcode: 2020A&A...638A...9R

Röser, Siegfried; Schilbach, Elena


Aims: Within a sphere of 400 pc radius around the Sun, we aim to search for members of the Pisces-Eridanus (Psc-Eri) stellar stream in the Gaia Data Release 2 data set. We compare basic astrophysical characteristics of the stream with those of the Pleiades.
Methods: We used a modified convergent-point method to identify stars with 2D vel…

2020 Astronomy and Astrophysics
Gaia 23
Systematic versus statistical uncertainties in masses and magnifications of the Hubble Frontier Fields
DOI: 10.1093/mnras/staa921 Bibcode: 2020MNRAS.494.4771R

Keeton, Charles R.; Raney, Catie A.; Brennan, Sean +1 more

The Hubble Frontier Fields data, along with multiple data sets obtained by other telescopes, have provided some of the most extensive constraints on cluster lenses to date. Multiple lens modelling teams analyzed the fields and made public a number of deliverables. By comparing these results, we can then undertake a unique and vital test of the sta…

2020 Monthly Notices of the Royal Astronomical Society
eHST 23
Multi-resolution Filtering: An Empirical Method for Isolating Faint, Extended Emission in Dragonfly Data and Other Low Resolution Images
DOI: 10.1088/1538-3873/ab9416 Bibcode: 2020PASP..132g4503V

van Dokkum, Pieter; Abraham, Roberto; Danieli, Shany +6 more

We describe an empirical, self-contained method to isolate faint, large-scale emission in imaging data of low spatial resolution. Multi-resolution filtering (MRF) uses independent data of superior spatial resolution and point source depth to create a model for all compact and high surface brightness objects in the field. This model is convolved wi…

2020 Publications of the Astronomical Society of the Pacific
eHST 23
Possible Production of Solar Spicules by Microfilament Eruptions
DOI: 10.3847/2041-8213/ab86a5 Bibcode: 2020ApJ...893L..45S

Yurchyshyn, Vasyl; Moore, Ronald L.; Sterling, Alphonse C. +1 more

We examine Big Bear Solar Observatory (BBSO) Goode Solar Telescope (GST) high spatial resolution (0"06), high-cadence (3.45 s), Hα-0.8 Å images of central-disk solar spicules, using data of Samanta et al. We compare with coronal-jet chromospheric-component observations of Sterling et al. Morphologically, bursts of spicules, referred to as "enhance…

2020 The Astrophysical Journal
Hinode 22