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Discovery of a highly eccentric, chromospherically active binary: ASASSN-V J192114.84+624950.8
DOI: 10.1093/mnras/stac1343 Bibcode: 2022MNRAS.514..200W

Kochanek, C. S.; Holoien, Thomas W. -S.; Stanek, K. Z. +5 more

As part of an All-Sky Automated Survey for SuperNovae (ASAS-SN) search for sources with large flux decrements, we discovered a transient where the quiescent, stellar source ASASSN-V J192114.84+624950.8 rapidly decreased in flux by $\sim 55{{\ \rm per\ cent}}$ (~0.9 mag) in the g band. The Transiting Exoplanet Survey Satellite light curve revealed …

2022 Monthly Notices of the Royal Astronomical Society
Gaia 3
Titan Stratospheric Haze Bands Observed in Cassini VIMS as Tracers of Meridional Circulation
DOI: 10.3847/PSJ/ac582d Bibcode: 2022PSJ.....3..114K

Le Mouélic, S.; Rodriguez, S.; Sotin, C. +9 more

We analyzed Cassini data to derive the nature and evolution of circumglobal annuli observed in the stratosphere of Titan, Saturn's largest moon. The annuli were observed between 2004 and 2017 in data acquired by the Visual and Infrared Mapping Spectrometer on board the Cassini spacecraft. We observed a north polar annulus, an equatorial annulus, a…

2022 The Planetary Science Journal
Cassini 3
Recent Formation of a Spiral Disk Hosting Progenitor Globular Clusters at the Center of the Perseus Brightest Cluster Galaxy. II. Progenitor Globular Clusters
DOI: 10.3847/1538-4357/ac4df6 Bibcode: 2022ApJ...927..138L

Ohyama, Youichi; Lim, Jeremy; Wong, Emily +1 more

We address the nature and origin of super star clusters (SSCs) discovered by Holtzman et al. within a radius of ~5 kpc from the center of NGC 1275, the giant elliptical galaxy at the center of the Perseus Cluster. We show that, in contrast with the much more numerous population of SSCs subsequently discovered up to ~30 kpc from the center of this …

2022 The Astrophysical Journal
eHST 3
Cloud-cloud collision and star formation in G323.18+0.15
DOI: 10.1051/0004-6361/202243317 Bibcode: 2022A&A...663A..97M

Li, Dalei; Tang, Xindi; Zhou, Jianjun +8 more

We studied the cloud-cloud collision candidate G323.18+0.15 based on signatures of induced filaments, clumps, and star formation. We used archival molecular spectrum line data from the SEDIGISM 13CO (J = 2−1) survey, from the Mopra southern Galactic plane CO survey, and infrared to radio data from the GLIMPSE, MIPS, Hi-GAL, and SGPS sur…

2022 Astronomy and Astrophysics
Herschel 3
The colibri telescope array for KBO detection through serendipitous stellar occultations: A technical description
DOI: 10.3389/fspas.2022.929573 Bibcode: 2022FrASS...9.9573M

Metchev, Stanimir; Pass, Emily; Mazur, Michael J. +4 more

We present the technical design, construction and testing of the Colibri telescope array at Elginfield Observatory near London, Ontario, Canada. Three 50-cm telescopes are arranged in a triangular array and are separated by 110–160 m. During operation, they will monitor field stars at the intersections of the ecliptic and galactic plane for serend…

2022 Frontiers in Astronomy and Space Sciences
Gaia 3
Pre-main sequence stars in LH 91
DOI: 10.1051/0004-6361/202243118 Bibcode: 2022A&A...663A..74C

Panagia, N.; Beccari, G.; De Marchi, G. +3 more


Aims: We study the accretion properties of pre-main sequence (PMS) low-mass stars in the LH 91 association within the Large Magellanic Clouds.
Methods: Using optical multiband photometry obtained with the Hubble Space Telescope, we identify 75 candidates showing Hα excess emission above the 3σ level with equivalent width EWHα

2022 Astronomy and Astrophysics
eHST 3
Optical Linear Polarization Study toward Czernik 3 Open Cluster at Different Spatial Scales
DOI: 10.3847/1538-3881/ac7445 Bibcode: 2022AJ....164...31U

Bisht, D.; Ganesh, Shashikiran; Uppal, Namita

We present the optical linear polarization observation of stars toward the core of the Czernik 3 cluster in the Sloan i band. The data were obtained using the EMPOL instrument on the 1.2 m telescope at Mount Abu Observatory. We study the dust distribution toward this cluster by combining the results from our polarization observations with the data…

2022 The Astronomical Journal
Gaia 3
Long-term Evolution of Postexplosion Helium-star Companions of Type Iax Supernovae
DOI: 10.3847/1538-4357/ac75bb Bibcode: 2022ApJ...933...65Z

Han, Zhanwen; McCully, Curtis; Heger, Alexander +3 more

Supernovae of Type Iax (SNe Iax) are an accepted faint subclass of hydrogen-free supernovae. Their origin, the nature of the progenitor systems, however, is an open question. Recent studies suggest that the weak deflagration explosion of a near-Chandrasekhar-mass white dwarf in a binary system with a helium-star donor could be the origin of SNe Ia…

2022 The Astrophysical Journal
eHST 3
Multispacecraft Remote Sensing and In Situ Observations of the 2020 November 29 Coronal Mass Ejection and Associated Shock: From Solar Source to Heliospheric Impacts
DOI: 10.3847/1538-4357/ac7ff6 Bibcode: 2022ApJ...937...44C

Liu, Ying D.; Zhu, Bei; Chen, Chong

We investigate the source eruption, propagation and expansion characteristics, and heliospheric impacts of the 2020 November 29 coronal mass ejection (CME) and associated shock, using remote sensing and in situ observations from multiple spacecraft. A potential-field source-surface model is employed to examine the coronal magnetic fields surroundi…

2022 The Astrophysical Journal
SOHO 3
Statistical properties of cataclysmic variables in the local galactic disc: a joint analysis of Gaia and XMM-Newton data
DOI: 10.1093/mnras/stac2354 Bibcode: 2022MNRAS.516.1263X

Wang, Q. Daniel; Xu, Xiao-jie; Li, Xiangdong

Cataclysmic variables (CVs) represent a key evolutionary phase of many low-mass stellar binaries and appear to collectively dominate the galactic X-ray background above ~1 keV. Statistical properties of CVs, however, remain poorly understood, even in the solar neighbourhood. We aim to obtain an X-ray luminosity-complete sample of local CVs whose d…

2022 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 3