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Binarity and beyond in A stars II. Disentangling the four stars in the vicinity of the triple HIP 87813 within the quintuple system HJ2814
DOI: 10.1093/mnras/stad873 Bibcode: 2023MNRAS.521.5255W

Katz, Boaz; Waisberg, Idel; Klein, Ygal

A-type stars are the progenitors of about half of the white dwarfs (WDs) that currently exist. The observational mappings of both multiplicities are far from complete and their connection is not known. We are in the process of obtaining tight constraints on a sample of 108 southern and nearby A-stars that are part of the VAST sample by conducting …

2023 Monthly Notices of the Royal Astronomical Society
Gaia Hipparcos 4
Eclipse timing variations in the WD + dM eclipsing binary RR Cae
DOI: 10.1093/mnras/stad1733 Bibcode: 2023MNRAS.523.5086R

Reichart, D. E.; Awiphan, S.; Haislip, J. B. +9 more

We present the binary model and the eclipse timing variations of the eclipsing binary RR Cae, which consists of a white dwarf eclipsed by an M-type dwarf companion. The multiwavelength optical photometry from the Transiting Exoplanet Survey Satellite (TESS), the 0.6-m PROMPT-8 telescope, and the 0.7-m Thai Robotic Telescope at Spring Brook Observa…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 4
How to improve our understanding of solar wind-magnetosphere interactions on the basis of the statistical evaluation of the energy budget in the magnetosheath?
DOI: 10.3389/fspas.2023.1163139 Bibcode: 2023FrASS..1063139V

Sorriso-Valvo, Luca; Plaschke, Ferdinand; Nakamura, Rumi +6 more

Solar wind (SW) quantities, referred to as coupling parameters (CPs), are often used in statistical studies devoted to the analysis of SW–magnetosphere–ionosphere couplings. Here, the CPs and their limitations in describing the magnetospheric response are reviewed. We argue that a better understanding of SW magnetospheric interactions could be ach…

2023 Frontiers in Astronomy and Space Sciences
Cluster 4
Distribution and dynamics of decimetre-sized dust agglomerates in the coma of 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stad032 Bibcode: 2023MNRAS.519.5775L

Agarwal, Jessica; Schröter, Matthias; Lemos, Pablo

We present a method to analyse images of the coma of 67P/Churyumov-Gerasimenko obtained using OSIRIS, the main imaging system on-board Rosetta, where dust aggregates can be seen as bright tracks because of their relative velocity with respect to the spacecraft. We applied this method to 105 images taken in 2015 July, 2015 December, and 2016 Januar…

2023 Monthly Notices of the Royal Astronomical Society
Rosetta 4
Machine learning detection of dust impact signals observed by the Solar Orbiter
DOI: 10.5194/angeo-41-69-2023 Bibcode: 2023AnGeo..41...69K

Mann, Ingrid; Vaverka, Jakub; Soucek, Jan +8 more

This article presents the results of automatic detection of dust impact signals observed by the Solar Orbiter - Radio and Plasma Waves instrument.

A sharp and characteristic electric field signal is observed by the Radio and Plasma Waves instrument when a dust particle impacts the spacecraft at high velocity. In this way, ∼ 5-20 dust impacts …

2023 Annales Geophysicae
SolarOrbiter 4
An Ongoing Tidal Capture in the Large Magellanic Cloud: The Low-mass Star Cluster KMK 88-10 Captured by the Massive Globular Cluster NGC 1835?
DOI: 10.3847/1538-4357/ace18e Bibcode: 2023ApJ...953..125G

Vesperini, Enrico; Cadelano, Mario; Pallanca, Cristina +6 more

In the context of a project aimed at characterizing the dynamical evolution of old globular clusters in the Large Magellanic Cloud, we have secured deep HST/WFC3 images of the massive cluster NGC 1835. In the field of view of the acquired images, at a projected angular separation of approximately 2' from the cluster, we detected the small stellar …

2023 The Astrophysical Journal
Gaia eHST 4
Three cases of optical periodic modulation in Active Galactic Nuclei
DOI: 10.1093/mnras/stad1168 Bibcode: 2023MNRAS.522.2928L

Wang, Zhongxiang; Li, Jie; Zheng, Dong

We report on the case of optical periodic modulation discovered in two Active Galactic Nuclei (AGN) and one candidate AGN. Analysing the archival optical data obtained from large transient surveys, namely the Catalina Real-Transient Survey (CRTS) and the Zwicky Transient Facility (ZTF), we find periodicities of 2169.7, 2103.1, and 1462.6 d in sour…

2023 Monthly Notices of the Royal Astronomical Society
XMM-Newton 4
BD +30°549: a young helium-weak silicon star in the NGC 1333 star-forming region
DOI: 10.1093/mnras/stad193 Bibcode: 2023MNRAS.520.1296P

Potravnov, I.; Ryabchikova, T.; Mashonkina, L.

We present results of the spectroscopic study of the chemically peculiar star BD +30°549, which is a bona fide member of the young NGC 1333 star-forming region. We found that the star possesses negligible rotation and a helium-weak spectroscopic pattern with strongly enhanced Si II and Si III lines. The fundamental parameters of the star, Tef…

2023 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 4
Three-stage Collapse of the Long Gamma-Ray Burst from GRB 160625B Prompt Multiwavelength Observations
DOI: 10.3847/1538-4357/ac9307 Bibcode: 2023ApJ...943..181L

Rebolo, R.; Lipunov, V. M.; Kornilov, V. G. +37 more

This article presents the early results of synchronous multiwavelength observations of one of the brightest gamma-ray bursts (GRBs) GRB 160625B with the detailed continuous fast optical photometry of its optical counterpart obtained by MASTER and with hard X-ray and gamma-ray emission, obtained by the Lomonosov and Konus-Wind spacecraft. The detai…

2023 The Astrophysical Journal
INTEGRAL 4
Faint but Not Forgotten. I. First Results from a Search for Astrospheres around AGB Stars in the Far-ultraviolet
DOI: 10.3847/1538-3881/acccf2 Bibcode: 2023AJ....165..229S

Sahai, Raghvendra; Stenger, Benjamin

Using the GALEX archive, we have discovered extended structures around ten asymptotic giant branch (AGB) stars (out of a total 92 searched) emitting in the far-ultraviolet (FUV) band. In all but one, we find the typical morphology expected for a spherical wind moving relative to, and interacting with, the interstellar medium (ISM) to produce an as…

2023 The Astronomical Journal
Gaia Herschel 4