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Observation of the Solar Corona Using Radio Scintillation with the Akatsuki Spacecraft: Difference Between Fast and Slow Wind
DOI: 10.1007/s11207-022-01968-9 Bibcode: 2022SoPh..297...34C

Matsumoto, Takuma; Pätzold, Martin; Imamura, Takeshi +8 more

The properties of the coronal plasma at heliocentric distances of 1.5 - 8.9 R (solar radii) were studied with radio-occultation observations using JAXA's Akatsuki spacecraft in 2016. Physical parameters that characterize the solar wind were retrieved from the intensity-scintillation time series by fitting a theoretical spectrum to the …

2022 Solar Physics
Hinode SOHO 9
Machine learning for fast transients for the Deeper, Wider, Faster programme with the Removal Of BOgus Transients (ROBOT) pipeline
DOI: 10.1093/mnras/stac983 Bibcode: 2022MNRAS.513.1742G

Mahabal, Ashish; Zhang, Jielai; Cooke, Jeff +3 more

The Deeper, Wider, Faster (DWF) programme is optimized to detect fast transients that show luminosity changes on time-scales of sub-second to days using fast cadence simultaneous observations and rapid response follow up. One of the significant bottlenecks in DWF is the time required to assess candidates for rapid follow up and to manually inspect…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 9
Spectral Evolution of Dark Asteroid Surfaces Induced by Space Weathering over a Decade
DOI: 10.3847/2041-8213/ac92e4 Bibcode: 2022ApJ...939L...9H

Hasegawa, Sunao; Marsset, Michaël; Im, Myungshin +20 more

The surfaces of airless bodies like asteroids in the solar system are known to be affected by space weathering. Experiments simulating space weathering are essential for studying the effects of this process on meteorite samples, but the problem is that the time spent to reproduce space weathering in these experiments is billions of times shorter t…

2022 The Astrophysical Journal
AKARI 9
Optical and near-infrared data and modelling of nova V5668 Sgr
DOI: 10.1093/mnras/stac097 Bibcode: 2022MNRAS.511.1591T

Lawrence, S. S.; Sokolovsky, K. V.; Diaz, M. +4 more

We present Hubble Space Telescope optical images, Keck-OSIRIS near-infrared (NIR) integral field spectroscopy data cubes and Keck-Near InfraRed Camera-2 (NIRC2) NIR images of nova V5668 Sgr from 2016 to 2019. The observations indicate enhanced emission at the polar caps and equatorial torus for low-ionization lines, and enhanced high-ionization em…

2022 Monthly Notices of the Royal Astronomical Society
eHST 9
Isolated Massive Star Formation in G28.20-0.05
DOI: 10.3847/1538-4357/ac90c7 Bibcode: 2022ApJ...939..120L

Law, Chi-Yan; Garay, Guido; Mardones, Diego +9 more

We report high-resolution 1.3 mm continuum and molecular line observations of the massive protostar G28.20-0.05 with Atacama Large Millimeter/submillimeter Array. The continuum image reveals a ring-like structure with 2000 au radius, similar to morphology seen in archival 1.3 cm Very Large Array observations. Based on its spectral index and associ…

2022 The Astrophysical Journal
Gaia Herschel eHST 9
A New Absolute Proper Motion Determination of Leo I Using HST/WFPC2 Images and Gaia EDR3
DOI: 10.3847/1538-3881/ac30dc Bibcode: 2022AJ....163....1C

Horch, Elliott P.; Kozhurina-Platais, Vera; Casetti-Dinescu, Dana I. +3 more

We measure the absolute proper motion of Leo I using a WFPC2/HST data set that spans up to 10 yr to date the longest time baseline utilized for this satellite. The measurement relies on ~2300 Leo I stars located near the center of light of the galaxy; the correction to absolute proper motion is based on 174 Gaia EDR3 stars and 10 galaxies. Having …

2022 The Astronomical Journal
Gaia eHST 9
Sublimation origin of active asteroid P/2018 P3
DOI: 10.1051/0004-6361/202244356 Bibcode: 2022A&A...666A.163K

Mutchler, Max; Jewitt, David; Agarwal, Jessica +4 more

Context. Active asteroids show (typically transient) cometary activity, driven by a range of processes. A sub-set, sometimes called main-belt comets, may be driven by sublimation and so could be useful for tracing the present-day distribution of asteroid ice. Object P/2018 P3 has a Tisserand parameter 3.096 but a high eccentricity 0.415, placing i…

2022 Astronomy and Astrophysics
eHST 9
KIC 2857323: A Double-mode High-amplitude δ Scuti Star with Amplitude Decline of the First Overtone Mode
DOI: 10.3847/1538-4357/ac86c9 Bibcode: 2022ApJ...936...48Y

Esamdin, Ali; Yang, Tao-Zhi; Zuo, Zhao-Yu +2 more

We investigate the pulsating behavior of KIC 2857323 using high-precision observations from the Kepler mission. Fourier analysis of 4 yr time-series data reveals five independent frequencies for the light variation. Among them, two strong frequencies f 1 and f 3 with a period ratio of 0.774 identify this star as a double-mode…

2022 The Astrophysical Journal
Gaia 9
The Galactic Distribution of Phosphorus: A Survey of 163 Disk and Halo Stars
DOI: 10.3847/1538-3881/ac77f8 Bibcode: 2022AJ....164...61M

Janowiecki, Steven; Cargile, Phillip; Hawkins, Keith +3 more

Phosphorus (P) is a critical element for life on Earth, yet the cosmic production sites of P are relatively uncertain. To understand how P has evolved in the solar neighborhood, we measured abundances for 163 FGK stars over a range of -1.09 < [Fe/H] < 0.47 using observations from the Habitable-zone Planet Finder instrument on the Hobby-Eberl…

2022 The Astronomical Journal
Gaia 9
Spatiokinematic models of five nova remnants: correlations between nova shell axial ratio, expansion velocity, and speed class
DOI: 10.1093/mnras/stac563 Bibcode: 2022MNRAS.512.2003S

Guerrero, M. A.; Toalá, J. A.; Santamaría, E. +3 more

We present long-slit intermediate-dispersion spectroscopic observations and narrow-band direct imaging of four classical nova shells, namely T Aur, HR Del, DQ Her, and QU Vul, and the nova-like source CK Vul. These are used to construct models of their nebular remnants using the morphokinematic modelling tool SHAPE to reveal their 3D shape. All th…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 9