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Disks and Outflows in the Intermediate-mass Star-forming Region NGC 2071 IR
DOI: 10.3847/1538-4357/ac7464 Bibcode: 2022ApJ...933..178C

Li, Zhi-Yun; Sheehan, Patrick D.; Megeath, S. Thomas +13 more

We present Atacama Large Millimeter Array band 6/7 (1.3 mm/0.87 mm) and Very Large Array Ka-band (9 mm) observations toward NGC 2071 IR, an intermediate-mass star-forming region. We characterize the continuum and associated molecular line emission toward the most luminous protostars, i.e., IRS1 and IRS3, on ~100 au (0.″2) scales. IRS1 is partly re…

2022 The Astrophysical Journal
Gaia 7
Searching for young runaways across the sky
DOI: 10.1093/mnras/stac2829 Bibcode: 2022MNRAS.517.1946K

Stassun, Keivan G.; Kounkel, Marina; Leigh, Nathan +1 more

We present a catalogue of 3354 candidate young stars within 500 pc that appear to have been ejected from their parent associations with relative speeds of >5 km s-1. These candidates have been homogeneously selected through performing a 2D spherical traceback of previously identified pre-main-sequence candidates to various star-formi…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
Kepler Pixel Project: Background RR Lyrae Stars in the Primary Kepler Mission Field of View
DOI: 10.3847/1538-4365/ac5e9e Bibcode: 2022ApJS..260...20F

Bódi, Attila; Szabó, Róbert; Forró, Adrienn +1 more

In this paper, we describe a project we initiated to investigate individual pixels in downloaded Kepler apertures in order to find objects in the background of the main targets with variable brightness. In the first paper of this series, we discovered and investigated 547 short-period eclipsing binaries. Here we present the independent discovery o…

2022 The Astrophysical Journal Supplement Series
Gaia 7
Revisiting Ulysses electron data with a triple fit of velocity distributions
DOI: 10.1051/0004-6361/202243477 Bibcode: 2022A&A...663A..67S

Fichtner, H.; Scherer, K.; Lazar, M. +1 more

Context. Given their uniqueness, the Ulysses data can still provide us with valuable new clues about the properties of plasma populations in the solar wind, and especially about their variations with heliographic coordinates. In the context of kinetic waves and instabilities in the solar wind plasma, the electron temperature anisotropy plays a cru…

2022 Astronomy and Astrophysics
Ulysses 7
Auroral kilometric radiation—The electron cyclotron maser paradigm
DOI: 10.3389/fspas.2022.1053303 Bibcode: 2022FrASS...953303B

Treumann, R. A.; Baumjohann, Wolfgang

Auroral kilometric radiation (AKR) is the paradigm of intense radio emission from planetary magnetospheres. Being close to the electron gyro frequency and/or its lower harmonics, its observation indicates the non-thermal state of the source plasma. Emission is produced when the plasma enters a state of energetic excitation which results in deforma…

2022 Frontiers in Astronomy and Space Sciences
Cluster 7
A Search for Predicted Astrometric Microlensing Events by Nearby Brown Dwarfs
DOI: 10.3847/1538-3881/ac9a41 Bibcode: 2022AJ....164..253L

Lu, Jessica R.; McGill, Peter; Leauthaud, Alexie +3 more

Gravitational microlensing has the potential to provide direct gravitational masses of single, free-floating brown dwarfs, independent of evolutionary and atmospheric models. The proper motions and parallaxes of nearby brown dwarfs can be used to predict close future alignments with distant background stars that cause a microlensing event. Targete…

2022 The Astronomical Journal
Gaia 7
K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant
DOI: 10.1093/mnras/stab3497 Bibcode: 2022MNRAS.510.5035S

Fridlund, M.; Guenther, E. W.; García, R. A. +29 more

We report new photometric and spectroscopic observations of the K2-99 planetary system. Asteroseismic analysis of the short-cadence light curve from K2's Campaign 17 allows us to refine the stellar properties. We find K2-99 to be significantly smaller than previously thought, with R = 2.55 ± 0.02 R. The new light curve also…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
Subarcsecond Imaging of a Solar Active Region Filament With ALMA and IRIS
DOI: 10.3389/fspas.2022.898115 Bibcode: 2022FrASS...9.8115D

Heinzel, P.; Gunár, S.; Leenaarts, J. +4 more

Quiescent filaments appear as absorption features on the solar disk when observed in chromospheric lines and at continuum wavelengths in the millimeter (mm) range. Active region (AR) filaments are their small-scale, low-altitude analogues, but they could not be resolved in previous mm observations. This spectral diagnostic can provide insight into…

2022 Frontiers in Astronomy and Space Sciences
Hinode IRIS 7
AMBITION - comet nucleus cryogenic sample return
DOI: 10.1007/s10686-021-09770-4 Bibcode: 2022ExA....54.1077B

Henri, Pierre; Bianchi, Eleonora; Codella, Claudio +27 more

We describe the AMBITION project, a mission to return the first-ever cryogenically-stored sample of a cometary nucleus, that has been proposed for the ESA Science Programme Voyage 2050. Comets are the leftover building blocks of giant planet cores and other planetary bodies, and fingerprints of Solar System's formation processes. We summarise some…

2022 Experimental Astronomy
Rosetta 7
Discovery of two bright high-redshift gravitationally lensed quasars revealed by Gaia
DOI: 10.1093/mnras/stab2960 Bibcode: 2022MNRAS.509..738D

McMahon, Richard G.; Auger, Matthew W.; Anguita, Timo +4 more

We present the discovery and preliminary characterisation of two high-redshift gravitationally lensed quasar systems in Gaia Data Release 2 (DR2). Candidates with multiple close-separation Gaia detections and quasar-like colours in WISE, Pan-STARRS, and DES are selected for follow-up spectroscopy with the New Technology Telescope. We confirm DES J…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7