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Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching
DOI: 10.3847/1538-4357/ac7051 Bibcode: 2022ApJ...933...30T

Matharu, Jasleen; Muzzin, Adam; van der Wel, Arjen +9 more

One of the challenges in understanding the quenching processes for galaxies is connecting progenitor star-forming populations to their descendant quiescent populations over cosmic time. Here we attempt a novel approach to this challenge by assuming that the underlying stellar mass distribution of galaxies is not significantly altered during enviro…

2022 The Astrophysical Journal
eHST 10
Quasar and galaxy classification using Gaia EDR3 and CatWise2020
DOI: 10.1051/0004-6361/202244859 Bibcode: 2022A&A...668A..99H

Bailer-Jones, Coryn A. L.; Hughes, Arvind C. N.; Jamal, Sara

In this work, we assess the combined use of Gaia photometry and astrometry with infrared data from CatWISE in improving the identification of extragalactic sources compared to the classification obtained using Gaia data. Here we perform a comprehensive study in which we assess different input feature configurations and prior functions to identify …

2022 Astronomy and Astrophysics
Gaia 10
IM Normae: The Death Spiral of a Cataclysmic Variable?
DOI: 10.3847/1538-4357/abec87 Bibcode: 2022ApJ...924...27P

Myers, Gordon; Monard, Berto; Dvorak, Shawn +18 more

We present a study of the orbital light curves of the recurrent nova IM Normae since its 2002 outburst. The broad "eclipses" recur with a 2.46 hr period, which increases on a timescale of 1.28(16) × 106 yr. Under the assumption of conservative mass transfer, this suggests a rate near 10-7 M yr-1, and t…

2022 The Astrophysical Journal
Gaia 10
SRGA J181414.6-225604: A New Galactic Symbiotic X-Ray Binary Outburst Triggered by an Intense Mass-loss Episode of a Heavily Obscured Mira Variable
DOI: 10.3847/1538-4357/ac7c6e Bibcode: 2022ApJ...935...36D

Soria, Roberto; Boyer, Martha L.; Conroy, Charlie +24 more

We present the discovery and multiwavelength characterization of SRGA J181414.6-225604, a Galactic hard X-ray transient discovered during the ongoing SRG/ART-XC sky survey. Using data from the Palomar Gattini-IR survey, we identify a spatially and temporally coincident variable infrared (IR) source, IRAS 18111-2257, and classify it as a very-late-…

2022 The Astrophysical Journal
AKARI Gaia INTEGRAL XMM-Newton 10
A 16 hr Transit of Kepler-167 e Observed by the Ground-based Unistellar Telescope Network
DOI: 10.3847/2041-8213/aca073 Bibcode: 2022ApJ...940L..39P

Esposito, Thomas M.; Wagner, Kevin; Dalba, Paul A. +35 more

More than 5000 exoplanets have been confirmed and among them almost 4000 were discovered by the transit method. However, few transiting exoplanets have an orbital period greater than 100 days. Here we report a transit detection of Kepler-167 e, a "Jupiter analog" exoplanet orbiting a K4 star with a period of 1071 days, using the Unistellar ground-…

2022 The Astrophysical Journal
Gaia 10
Tidal Quality of the Hot Jupiter WASP-12b
DOI: 10.3390/universe8040211 Bibcode: 2022Univ....8..211E

Makarov, Valeri V.; Efroimsky, Michael

WASP-12b stands out among the planets of its class of hot Jupiters because of the observed fast orbital decay attributed to tidal dissipation. The measured rate of the orbital period change is Pṡorb=‑29±3ms/yr= ‑(9.2±1.0)×10‑10s/s. In the literature heretofore, all attempts to explain this high rate were based on the assumption that the orbital ev…

2022 Universe
Gaia 10
The peculiar abundances of HE 1005-1439. A carbon-enhanced extremely metal-poor star contaminated with products of both s- and i-process nucleosynthesis
DOI: 10.1051/0004-6361/202141775 Bibcode: 2022A&A...657A..50G

Goswami, Aruna; Goswami, Partha Pratim

Context. Understanding the surface chemical composition of carbon-enhanced metal-poor (CEMP) stars with enhanced abundances of heavy elements remains problematic.
Aims: One of the primary objectives is to investigate the origin of the peculiar abundance pattern observed in the carbon-enhanced extremely metal-poor object HE 1005-1439, which is…

2022 Astronomy and Astrophysics
Gaia 10
Improved Modeling of Mars' HDO Cycle Using a Mars' Global Climate Model
DOI: 10.1029/2022JE007192 Bibcode: 2022JGRE..12707192V

Montmessin, Franck; Trokhimovskiy, Alexander; Korablev, Oleg +11 more

HDO and the D/H ratio are essential to understand Mars past and present climate, in particular with regard to the evolution through ages of the Martian water cycle. We present here new modeling developments of the HDO cycle with the Laboratoire de Météorologie Dynamique Mars Global Climate Model (GCM). The present study aims at exploring the behav…

2022 Journal of Geophysical Research (Planets)
ExoMars-16 10
Plausibility of ultraviolet burst generation in the low solar chromosphere
DOI: 10.1051/0004-6361/202243304 Bibcode: 2022A&A...665A.116N

Cheng, Guanchong; Ni, Lei; Lin, Jun

Context. Ultraviolet (UV) bursts and Ellerman bombs (EBs) are small-scale magnetic reconnection events taking place in the highly stratified, low solar atmosphere. The plasma density, reconnection mechanisms, radiative cooling and transfer processes clearly differ from one layer of the atmosphere to the next. In particular, EBs are believed to for…

2022 Astronomy and Astrophysics
IRIS 10
Radio Jet Proper-motion Analysis of Nine Distant Quasars above Redshift 3.5
DOI: 10.3847/1538-4357/ac87f8 Bibcode: 2022ApJ...937...19Z

Frey, Sándor; Gabányi, Krisztina Éva; An, Tao +2 more

Up to now, jet kinematic studies of radio quasars have barely reached beyond the redshift range z > 3.5. This significantly limits our knowledge of high-redshift jets, which can provide key information for understanding the jet nature and the growth of black holes in the early universe. In this paper, we selected nine radio-loud quasars at z &g…

2022 The Astrophysical Journal
Gaia 10