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Lens parameters for Gaia18cbf - a long gravitational microlensing event in the Galactic plane
DOI: 10.1051/0004-6361/202142602 Bibcode: 2022A&A...662A..59K

Mróz, P.; Gromadzki, M.; Narita, N. +29 more

Context. The timescale of a microlensing event scales as a square root of a lens mass. Therefore, long-lasting events are important candidates for massive lenses, including black holes.
Aims: Here, we present the analysis of the Gaia18cbf microlensing event reported by the Gaia Science Alerts system. It exhibited a long timescale and features…

2022 Astronomy and Astrophysics
Gaia 13
Nebular-phase spectra of Type Ia supernovae from the Las Cumbres Observatory Global Supernova Project
DOI: 10.1093/mnras/stac192 Bibcode: 2022MNRAS.511.3682G

Wheeler, J. C.; Galbany, L.; Howell, D. A. +17 more

The observed diversity in Type Ia supernovae (SNe Ia) - the thermonuclear explosions of carbon-oxygen white dwarf stars used as cosmological standard candles - is currently met with a variety of explosion models and progenitor scenarios. To help improve our understanding of whether and how often different models contribute to the occurrence of SNe…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
Revealing the Nature of a Lyα Halo in a Strongly Lensed Interacting System at z = 2.92
DOI: 10.3847/1538-4357/ac7c1a Bibcode: 2022ApJ...935...17S

Rigby, Jane R.; Sharon, Keren; Infante, Leopoldo +12 more

Spatially extended halos of H I Lyα emission are now ubiquitously found around high-redshift star-forming galaxies. But our understanding of the nature and powering mechanisms of these halos is still hampered by the complex radiative transfer effects of the Lyα line and limited angular resolution. In this paper, we present resolved Multi Unit Spec…

2022 The Astrophysical Journal
Gaia eHST 13
Two Candidate KH 15D-like Systems from the Zwicky Transient Facility
DOI: 10.3847/2041-8213/ac7b2d Bibcode: 2022ApJ...933L..21Z

Fang, Min; Zang, Weicheng; Dong, Subo +8 more

KH 15D contains a circumbinary disk that is tilted relative to the orbital plane of the central binary. The precession of the disk and the orbital motion of the binary together produce rich phenomena in the photometric light curve. In this work, we present the discovery and preliminary analysis of two objects that resemble the key features of KH 1…

2022 The Astrophysical Journal
Gaia 13
The Rapidly Evolving Asymptotic Giant Branch Star, V Hya: ALMA Finds a Multiring Circus with High-velocity Outflows
DOI: 10.3847/1538-4357/ac568a Bibcode: 2022ApJ...929...59S

Sahai, R.; Morris, M. R.; Lee, C. -F. +3 more

We have observed the mass-losing carbon star V Hya that is apparently transitioning from an asymptotic giant branch star to a bipolar planetary nebula, at an unprecedented angular resolution of ~0.″4-0.″6 with the Atacama Large Millimeter/submillimeter Array. Our 13CO and 12CO (J = 3-2 and J = 2-1) images have led to the disc…

2022 The Astrophysical Journal
Gaia 13
ALMA Detections of [O III] and [C II] Emission Lines From A1689-zD1 at z = 7.13
DOI: 10.3847/1538-4357/ac5cc7 Bibcode: 2022ApJ...929..161W

Hashimoto, Tetsuya; Goto, Tomotsugu; Kim, Seong Jin +10 more

A1689-zD1 is one of the most distant galaxies, discovered with the aid of gravitational lensing, providing us with an important opportunity to study galaxy formation in the very early universe. In this study, we report the detection of [C II]158 µm and [O III]88 µm emission lines of A1689-zD1 in the Atacama Large Millimeter/submillimet…

2022 The Astrophysical Journal
eHST 13
Characterization of hot populations of Melotte 66 open cluster using Swift/UVOT
DOI: 10.1093/mnras/stac2241 Bibcode: 2022MNRAS.516.2444R

Subramaniam, Annapurni; Panthi, Anju; Vaidya, Kaushar +3 more

Ultraviolet (UV) wavelength observations have made a significant contribution to our understanding of hot stellar populations of star clusters. Multiwavelength spectral energy distributions (SEDs) of stars, including ultraviolet observations, have proven to be an excellent tool for discovering unresolved hot companions in exotic stars such as blue…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
Phase spirals in cosmological simulations of Milky Way-sized galaxies
DOI: 10.1093/mnras/stab3417 Bibcode: 2022MNRAS.510..154G

Antoja, T.; Ramos, P.; García-Conde, B. +2 more

We study the vertical perturbations in the galactic disc of the Milky Way-size high-resolution hydrodynamical cosmological simulation named GARROTXA. We detect phase spirals in the vertical projection Z - VZ of disc's stellar particles for the first time in this type of simulations. Qualitatively similar structures were detected in the …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 13
The Rotation of Magnetic Flux Ropes Formed during Solar Eruption
DOI: 10.3847/2041-8213/ac5740 Bibcode: 2022ApJ...927L..14Z

Wang, Yuming; Liu, Rui; Jiang, Chaowei +3 more

Eruptions of solar filaments often show rotational motion about their rising direction, but the mechanism governing such rotation, and how the rotation is related to the initial morphology of the preeruptive filament (and cospatial sigmoid), filament chirality, and magnetic helicity, remains elusive. The conventional view of rotation as a result o…

2022 The Astrophysical Journal
Hinode 13
Modeling the Transport of Relativistic Solar Protons along a Heliospheric Current Sheet during Historic GLE Events
DOI: 10.3847/1538-4357/ac795d Bibcode: 2022ApJ...934...82W

Laitinen, Timo; Dalla, Silvia; Waterfall, Charlotte O. G. +2 more

There are many difficulties associated with forecasting high-energy solar particle events at Earth. One issue is understanding why some large solar eruptive events trigger ground-level enhancement (GLE) events and others do not. In this work we perform 3D test particle simulations of a set of historic GLEs to understand more about what causes thes…

2022 The Astrophysical Journal
SOHO 13