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The Dynamic Coupling of Streamers and Pseudostreamers to the Heliosphere
DOI: 10.3847/1538-4357/ac5d5b Bibcode: 2022ApJ...929..185A

Antiochos, S. K.; Higginson, A. K.; Wyper, P. F. +3 more

The slow solar wind is generally believed to result from the interaction of open and closed coronal magnetic flux at streamers and pseudostreamers. We use three-dimensional magnetohydrodynamic simulations to determine the detailed structure and dynamics of open-closed interactions that are driven by photospheric convective flows. The photospheric …

2022 The Astrophysical Journal
SolarOrbiter 5
Observed Rate Variations in Superflaring G-type Stars
DOI: 10.3847/1538-4357/aca476 Bibcode: 2022ApJ...941..193C

Yang, Kai; Crowley, James; Wheatland, Michael S.

Flare occurrence on the Sun is highly variable, exhibiting both short-term variation due to the emergence and evolution of active regions, and long-term variation from the solar cycle. On solar-like stars, more energetic stellar flares (superflares) have been observed, and it is of interest to determine whether the observed rates of superflare occ…

2022 The Astrophysical Journal
Gaia 5
Detection of spicules termed rapid blueshifted excursions as seen in the chromosphere via H α and the transition region via Si IV 1394 Å line emission
DOI: 10.1093/mnras/stac1895 Bibcode: 2022MNRAS.515.2672V

Shetye, Juie; Doyle, J. Gerry; Vilangot Nhalil, Nived

We show signatures of spicules termed rapid blueshifted excursions (RBEs) in the Si IV 1394 Å emission line using a semi-automated detection approach. We use the H α filtergrams obtained by the CRISP imaging spectropolarimeter on the Swedish 1-m Solar Telescope and co-aligned Interface Region Imaging Spectrograph data using the SJI 1400 Å channel …

2022 Monthly Notices of the Royal Astronomical Society
IRIS 5
A Ghost in Boötes: The Least-Luminous Disrupted Dwarf Galaxy
DOI: 10.3847/1538-4357/ac9b4b Bibcode: 2022ApJ...940..127C

Conroy, Charlie; Ting, Yuan-Sen; Cargile, Phillip A. +9 more

We report the discovery of Specter, a disrupted ultrafaint dwarf galaxy revealed by the H3 Spectroscopic Survey. We detected this structure via a pair of comoving metal-poor stars at a distance of 12.5 kpc, and further characterized it with Gaia astrometry and follow-up spectroscopy. Specter is a 25° × 1° stream of stars that is entirely invisible…

2022 The Astrophysical Journal
Gaia 5
External or internal companion exciting the spiral arms in CQ Tau?
DOI: 10.1093/mnras/stac2119 Bibcode: 2022MNRAS.515.6109H

Testi, Leonardo; Benisty, Myriam; Pinte, Christophe +9 more

We present new high-contrast images in near-infrared wavelengths (λc = 1.04, 1.24, 1.62, 2.18, and 3.78 µm) of the young variable star CQ Tau, aiming to constrain the presence of companions in the protoplanetary disc. We reached a Ks-band contrast of 14 mag with SPHERE/IRDIS at separations greater than 0${_{.}^{\prime\prime}}$4 fr…

2022 Monthly Notices of the Royal Astronomical Society
Gaia eHST 5
Massive young stellar objects in the Local Group spiral galaxy M 33 identified using machine learning
DOI: 10.1093/mnras/stac2692 Bibcode: 2022MNRAS.517..140K

van Loon, Jacco Th; Oliveira, Joana M.; Kinson, David A.

We present a supervised machine learning classification of stellar populations in the Local Group spiral galaxy M 33. The Probabilistic Random Forest (PRF) methodology, previously applied to populations in NGC 6822, utilizes both near and far-IR classification features. It classifies sources into nine target classes: young stellar objects (YSOs), …

2022 Monthly Notices of the Royal Astronomical Society
Gaia Herschel 5
The Hubble PanCET Program: Emission Spectrum of Hot Jupiter HAT-P-41b
DOI: 10.3847/1538-3881/ac58fc Bibcode: 2022AJ....163..190F

Deming, Drake; Mikal-Evans, Thomas; Sing, David K. +7 more

We present the most complete emission spectrum for inflated hot Jupiter HAT-P-41b combining new Hubble Space Telescope Wide Field Camera/G141 spectrum from the Hubble Panchromatic Comparative Exoplanet Treasury program with archival Spitzer eclipse observations. We found a near blackbody-like emission spectrum, which is best fitted with an isother…

2022 The Astronomical Journal
eHST 5
On the origin of core radio emissions from black hole sources in the realm of relativistic shocked accretion flow
DOI: 10.1093/mnras/stac1398 Bibcode: 2022MNRAS.514.1940D

Stalin, C. S.; Rakshit, Suvendu; Nandi, Anuj +5 more

We study the relativistic, inviscid, advective accretion flow around the black holes and investigate a key feature of the accretion flow, namely the shock waves. We observe that the shock-induced accretion solutions are prevalent and such solutions are commonly obtained for a wide range of the flow parameters, such as energy (${\cal E}$) and angul…

2022 Monthly Notices of the Royal Astronomical Society
XMM-Newton 5
NGTS-21b: an inflated Super-Jupiter orbiting a metal-poor K dwarf
DOI: 10.1093/mnras/stac2884 Bibcode: 2022MNRAS.517.4447A

Wheatley, Peter J.; Bayliss, Daniel; Worters, Hannah L. +29 more

We report the discovery of NGTS-21b , a massive hot Jupiter orbiting a low-mass star as part of the Next Generation Transit Survey (NGTS). The planet has a mass and radius of 2.36 ± 0.21 MJ and 1.33 ± 0.03 RJ, and an orbital period of 1.543 d. The host is a K3V (Teff = 4660 ± 41 K) metal-poor ([Fe/H] = -0.26 ± 0.07…

2022 Monthly Notices of the Royal Astronomical Society
Gaia 5
TUVOpipe: A pipeline to search for UV transients with Swift-UVOT
DOI: 10.1051/0004-6361/202142997 Bibcode: 2022A&A...663A...5M

Wijnands, Rudy; Modiano, David; Parikh, Aastha +3 more

Despite the prevalence of transient-searching facilities operating across most wavelengths, the ultraviolet (UV) transient sky remains to be systematically studied. Therefore, we recently initiated the Transient Ultraviolet Objects (TUVO) project, with which we search for serendipitous UV transients in data obtained using currently available UV in…

2022 Astronomy and Astrophysics
Gaia XMM-Newton 5