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V0644 Ser: An Active Ultrashort Period Contact Binary Star
DOI: 10.1088/1674-4527/ac4ca5 Bibcode: 2022RAA....22c5024X

Zhu, Li-Ying; Xu, Hu-Shan; Thawicharat, Sarotsakulchai +1 more

The photometric solutions of the ultrashort period close binary V0644 Ser based on our new complete BVRI light curves are derived by the Wilson-Devininney code. The results show that V0644 Ser is a W-type shallow contact binary, and the third light was found in the R and I bands. Compared with the light curves in 2011, the amplitude variation of t…

2022 Research in Astronomy and Astrophysics
Gaia 7
Validation and Interpretation of a Three-dimensional Configuration of a Magnetic Cloud Flux Rope
DOI: 10.3847/1538-4357/ac7803 Bibcode: 2022ApJ...934...50H

Qiu, Jiong; Hu, Qiang; Jian, Lan K. +3 more

One strong magnetic cloud (MC) with a magnetic field magnitude reaching ~40 nT at 1 au during 2012 June 16-17 is examined in association with a preexisting magnetic flux rope (MFR) identified on the Sun. The MC is characterized by a quasi-three-dimensional (3D) flux rope model based on in situ measurements from the Wind spacecraft. The contents of…

2022 The Astrophysical Journal
SOHO VenusExpress 7
News from Gaia on σ Ori E: A case study for the wind magnetic braking process
DOI: 10.1051/0004-6361/202141512 Bibcode: 2022A&A...657A..60S

Eggenberger, P.; Meynet, G.; Mowlavi, N. +8 more

Context.σ Ori E, a massive helium B-type star, shows high surface rotation and a strong surface magnetic field, potentially challenging the process of wind magnetic braking.
Aims: The Gaia satellite provides an accurate distance to σ Ori E and confirms its membership to the σ Ori cluster. We account for these two key pieces of information in …

2022 Astronomy and Astrophysics
Gaia 7
Dynamical orbital evolution scenarios of the wide-orbit eccentric planet HR 5183b
DOI: 10.1093/mnras/stab3174 Bibcode: 2022MNRAS.509.3616M

Blunt, Sarah; Mustill, Alexander J.; Davies, Melvyn B. +1 more

The recently discovered giant exoplanet HR5183b exists on a wide, highly eccentric orbit (a = 18 au, e = 0.84). Its host star possesses a common proper-motion companion which is likely on a bound orbit. In this paper, we explore scenarios for the excitation of the eccentricity of the planet in binary systems such as this, considering planet-planet…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 7
Superflares on solar-like stars. A new method for identifying the true flare sources in photometric surveys
DOI: 10.1051/0004-6361/202244422 Bibcode: 2022A&A...668A.167V

Solanki, S. K.; Shapiro, A. I.; Usoskin, I. +5 more

Context. Over the past years, thousands of stellar flares have been detected by harvesting data from large photometric surveys. These detections, however, do not account for potential sources of contamination such as background stars or small Solar System objects appearing in the same aperture as the primary target.
Aims: We present a new met…

2022 Astronomy and Astrophysics
Gaia 7
Further Evidence for the Minifilament-eruption Scenario for Solar Polar Coronal Jets
DOI: 10.3847/1538-4357/ac473e Bibcode: 2022ApJ...927...79B

Savcheva, Antonia; Moore, Ronald L.; Savage, Sabrina L. +4 more

We examine a sampling of 23 polar-coronal-hole jets. We first identified the jets in soft X-ray (SXR) images from the X-ray telescope (XRT) on the Hinode spacecraft, over 2014-2016. During this period, frequently the polar holes were small or largely obscured by foreground coronal haze, often making jets difficult to see. We selected 23 jets among…

2022 The Astrophysical Journal
Hinode 7
On measuring the Hubble constant with X-ray reverberation mapping of active galactic nuclei
DOI: 10.1093/mnras/stab2950 Bibcode: 2022MNRAS.509..619I

Ingram, Adam; García, Javier A.; Kara, Erin +8 more

We show that X-ray reverberation mapping can be used to measure the distance to type 1 active galactic nuclei (AGNs). This is because X-ray photons originally emitted from the 'corona' close to the black hole irradiate the accretion disc and are reemitted with a characteristic 'reflection' spectrum that includes a prominent ~6.4 keV iron emission …

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 7
CLusters in the UV as EngineS (CLUES). I. Survey Presentation and FUV Spectral Analysis of the Stellar Light
DOI: 10.3847/1538-3881/ac9311 Bibcode: 2022AJ....164..208S

Hayes, Matthew; Chisholm, John; Östlin, Göran +18 more

The CLusters in the Uv as EngineS (CLUES) survey is a Cosmic Origins Spectrograph (COS) campaign aimed at acquiring the 1130-1770 Å rest-frame spectroscopy of very young (<20 Myr) and massive (>104 M ) star clusters in galaxies that are part of the Hubble treasury program Legacy ExtraGalactic UV Survey. In this first p…

2022 The Astronomical Journal
eHST 7
A Morphological Study of Galaxies Hosting Optical Variability-selected AGNs in the COSMOS Field
DOI: 10.3847/1538-4357/ac3edb Bibcode: 2022ApJ...925..157Z

Inoue, Akio K.; Yamada, Toru; Zhong, Yuxing +1 more

Morphological studies are crucial to investigate the connections between active galactic nucleus (AGN) activities and the evolution of galaxies. Substantial studies have found that radiative-mode AGNs primarily reside in disk galaxies, questioning the merger-driven mechanism of AGN activities. In this study, through Sérsic profile fitting and nonp…

2022 The Astrophysical Journal
AKARI eHST 7
Testing the Potential for Radio Variability in Disks around T Tauri Stars with Observations and Chemical Modeling
DOI: 10.3847/1538-4357/ac365a Bibcode: 2022ApJ...924..104E

Calvet, N.; D'Alessio, P.; Macías, E. +5 more

A multiwavelength observing campaign of the T Tauri star (TTS) GM Aur was undertaken in 2019 December. This campaign obtained Swift X-ray and NUV fluxes, HST NUV spectra, LCOGT ${u}^{{\prime} }> ${g}^{{\prime} }> ${r}^{{\prime} }> ${i}^{{\prime} }> and TESS photometry, CHIRON Hα spectra, Atacama Large Millimeter/submillimeter Array (AL…

2022 The Astrophysical Journal
eHST 7