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High-velocity CP2 stars in the Galactic halo
DOI: 10.1051/0004-6361/202245464 Bibcode: 2023A&A...674A.215F

Paunzen, E.; Prišegen, M.; Faltová, N. +2 more

Context. The second subclass of chemically peculiar stars, the CP2 stars, are early-type stars exhibiting anomalous abundances with variable line strengths possibly also accompanied by photometric variability that typically belong to the Galactic disk. However, a small fraction of these objects were recently found to be located far from the Galact…

2023 Astronomy and Astrophysics
Gaia 3
Multiwavelength study of radio galaxy Pictor A: detection of western hotspot in far-UV and possible origin of high energy emissions
DOI: 10.1093/mnras/stad716 Bibcode: 2023MNRAS.521.2704G

Stalin, C. S.; Sreekumar, P.; Bhattacharya, Debbijoy +2 more

A comprehensive study of the nucleus and western hotspot of Pictor A is carried out using AstroSat observations, 13 yr of Fermi, and archival Swift observations along with other published data. We report the first detection of the western hotspot of Pictor A in the far-UV band using observations from AstroSat-UVIT. The broad-band SED of the wester…

2023 Monthly Notices of the Royal Astronomical Society
Gaia XMM-Newton 3
Searching for quasi-periodic eruptions using machine learning
DOI: 10.1093/rasti/rzad015 Bibcode: 2023RASTI...2..238W

Young, A. J.; Webbe, Robbie

Quasi-periodic eruption (QPE) is a rare phenomenon in which the X-ray emission from the nuclei of galaxies shows a series of large amplitude flares. Only a handful of QPEs have been observed but the possibility remains that there are as yet undetected sources in archival data. Given the volume of data available a manual search is not feasible, and…

2023 RAS Techniques and Instruments
XMM-Newton 3
Third Epoch HST Imaging of a Nonradiative Shock in the Cygnus Loop Supernova Remnant
DOI: 10.3847/1538-4357/acc860 Bibcode: 2023ApJ...948...97S

Blair, William P.; Raymond, John C.; Sankrit, Ravi

We present new HST/WFC3 optical images of a region in the northeastern part of the Cygnus Loop supernova remnant, which includes a well-studied Balmer-line filament. These data represent the third epoch of HST Hα imaging and a second epoch of [O III] λ5007 imaging of that particular filament. The Hα images were used to measure the proper motions a…

2023 The Astrophysical Journal
eHST 3
TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPS
DOI: 10.1051/0004-6361/202245607 Bibcode: 2023A&A...671L...8B

Alonso, R.; Deleuil, M.; Erikson, A. +89 more

Context. TOI-1055 is a Sun-like star known to host a transiting Neptune-sized planet on a 17.5-day orbit (TOI-1055 b). Radial velocity (RV) analyses carried out by two independent groups using nearly the same set of HARPS spectra have provided measurements of planetary masses that differ by ∼2σ.
Aims: Our aim in this work is to solve the inco…

2023 Astronomy and Astrophysics
CHEOPS Gaia 3
The First Photometric and Spectroscopic Study of Contact Binary V2840 Cygni
DOI: 10.1088/1674-4527/acae6e Bibcode: 2023RAA....23b5017P

Jagirdar, Rukmini; Devarapalli, Shanti Priya; Pothuneni, Ravi Raja

The first photometric, spectroscopic and period variation studies of neglected short-period eclipsing binary V2840 Cygni are presented. High mass ratio contact binaries (HMRCBs), especially those in the weak-contact configuration, are vital when probing the evolutionary models of contact binaries (CBs) using stellar parameters. The photometric sol…

2023 Research in Astronomy and Astrophysics
Gaia 3
Low NH3/H2O ratio in comet C/2020 F3 (NEOWISE) at 0.7 au from the Sun
DOI: 10.1051/0004-6361/202346402 Bibcode: 2023A&A...677A.157D

McGuire, Brett A.; Drozdovskaya, Maria N.; Opitom, Cyrielle +7 more

Context. A lower-than-solar elemental nitrogen content has been demonstrated for several comets, including 1P/Halley and 67P/Churyumov-Gerasimenko (67P/C-G) with independent in situ measurements of volatile and refractory budgets. The recently discovered semi-refractory ammonium salts in 67P/C-G are thought to be the missing nitrogen reservoir in …

2023 Astronomy and Astrophysics
Rosetta 3
TOI-858 B b: A hot Jupiter on a polar orbit in a loose binary
DOI: 10.1051/0004-6361/202244940 Bibcode: 2023A&A...679A..70H

Bouchy, F.; Stassun, K.; Winn, J. N. +31 more

We report the discovery of a hot Jupiter on a 3.28-day orbit around a 1.08 M G0 star that is the secondary component in a loose binary system. Based on follow-up radial velocity observations of TOI-858 B with CORALIE on the Swiss 1.2 m telescope and CHIRON on the 1.5 m telescope at the Cerro Tololo Inter-American Observatory (CTIO), we…

2023 Astronomy and Astrophysics
Gaia Hipparcos 3
A deep dive into the Type II globular cluster NGC 1851
DOI: 10.1093/mnras/stad2950 Bibcode: 2023MNRAS.526.2960D

Milone, A. P.; Cordoni, G.; Marino, A. F. +13 more

About one-fifth of the Galactic globular clusters (GCs), dubbed Type II GCs, host distinct stellar populations with different heavy elements abundances. NGC 1851 is one of the most studied Type II GCs, surrounded by several controversies regarding the spatial distribution of its populations and the presence of star-to-star [Fe/H], C+N+O, and age d…

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST 3
The Second International Asteroid Warning Network Timing Campaign: 2005 LW3
DOI: 10.3847/PSJ/acfd22 Bibcode: 2023PSJ.....4..203F

Licandro, Javier; Granvik, Mikael; Thuillot, William +90 more

The Earth close approach of near-Earth asteroid 2005 LW3 on 2022 November 23 represented a good opportunity for a second observing campaign to test the timing accuracy of astrometric observation. With 82 participating stations, the International Asteroid Warning Network collected 1046 observations of 2005 LW3 around the time of the close approach.…

2023 The Planetary Science Journal
Gaia 3