Search Publications

Ups and downs in the X-ray emission of the colliding wind binaries HD 168112 and HD 167971
DOI: 10.1051/0004-6361/202450158 Bibcode: 2024A&A...687A.197R

Blomme, R.; Nazé, Y.; Rauw, G. +2 more

Context. The long-period O-star binary system HD 168112 and the triple O-star system HD 167971 are well-known sources of non-thermal radio emission that arises from a colliding wind interaction. The wind-wind collisions in these systems should result in phase-dependent X-ray emissions. The presence of a population of relativistic electrons in the …

2024 Astronomy and Astrophysics
XMM-Newton 1
Mutual occurrence ratio of planets - I. New clues to reveal origins of hot and warm Jupiter from the RV sample
DOI: 10.1093/mnras/stae733 Bibcode: 2024MNRAS.529.3958S

Zhang, Hui; Zhou, Ji-Lin; Su, Xiang-Ning

Many studies have analysed planetary occurrence rates and their dependence on the host's properties to provide clues to planet formation, but few have focused on the mutual occurrence ratio of different kinds of planets. Such relations reveal whether and how one type of planet evolves into another, e.g. from a cold Jupiter (CJ) to a warm Jupiter (…

2024 Monthly Notices of the Royal Astronomical Society
Gaia 1
The ESO-VLT MIKiS survey reloaded: The internal kinematics of the core of M75
DOI: 10.1051/0004-6361/202450147 Bibcode: 2024A&A...688A.133L

Vesperini, Enrico; Cadelano, Mario; Pallanca, Cristina +7 more

We present the results of a study aimed at characterizing the kinematics of the inner regions of the halo globular cluster M75 (NGC 6864) based on data acquired as part of the ESO-VLT Multi-Instrument Kinematic Survey (MIKiS) of Galactic globular clusters. Our analysis includes the first determination of the line-of-sight velocity dispersion profi…

2024 Astronomy and Astrophysics
Gaia eHST 1
The outskirts of M33: Tidally induced distortions versus signatures of gas accretion
DOI: 10.1051/0004-6361/202348910 Bibcode: 2024A&A...685A..38C

Burkert, Andreas; Corbelli, Edvige


Aims: We investigate a possible close encounter between M33 and M31 in the past to understand the role of galaxy-galaxy interactions in shaping the matter distribution in galaxy outskirts.
Methods: By examining a variety of initial conditions, we recovered possible orbital trajectories of M33, M31, and the Milky Way in the past, which ar…

2024 Astronomy and Astrophysics
eHST 1
Astronomical Test with CMOS on the 60 cm Telescope at the Xinglong Observatory, NAOC
DOI: 10.1088/1674-4527/ad359a Bibcode: 2024RAA....24e5009M

Fan, Zhou; Zhang, Yu; Wu, Hong +2 more

This work shows details of an evaluation of an observational system comprising a complementary metal-oxide-semiconductor detector, 60 cm telescope and filter complement. The system's photometric precision and differential photometric precision, and extinction coefficients were assessed through observations of Supersky flat fields, open clusters, s…

2024 Research in Astronomy and Astrophysics
Gaia 1
The Origin of High-velocity Stars Considering the Impact of the Large Magellanic Cloud
DOI: 10.3847/1538-3881/ad18c4 Bibcode: 2024AJ....167...76L

Shi, Jianrong; Huang, Yang; Ma, Jun +5 more

Utilizing astrometric parameters sourced from Gaia Data Release 3 and radial velocities obtained from various spectroscopic surveys, we identify 519 high-velocity stars (HiVels) with a total velocity in the Galactocentric rest frame greater than 70% of their local escape velocity under the Gala MilkyWayPotential. Our analysis reveals that the majo…

2024 The Astronomical Journal
Gaia 1
Detection of the [C I] λ8727 emission line. Low-ionization structures in NGC 7009
DOI: 10.1051/0004-6361/202450325 Bibcode: 2024A&A...689A..14A

Boumis, P.; Walsh, J. R.; Akras, S. +5 more

We report the first spatially resolved detection of the near-infrared [C I] λ8727 emission from the outer pair of low-ionization structures in the planetary nebula NGC 7009 from data obtained by the Multi Unit Spectroscopic Explorer integral field unit. This atomic carbon emission marks the transition zone between ionized and neutral gas and for t…

2024 Astronomy and Astrophysics
Gaia 1
Study of a Red Clump Giant, KIC 11087027, with High Rotation and Strong Infrared Excess—Evidence of Tidal Interaction for High Lithium Abundance
DOI: 10.3847/2041-8213/ad62f6 Bibcode: 2024ApJ...971L...3S

Zhao, Gang; Reddy, Bacham E.; Pandey, Jeewan C. +2 more

This Letter presents results from Kepler photometric light curves and a high-resolution spectroscopic study of a super-Li-rich giant KIC11087027. Using the light-curve analysis, we measured the star's rotational period P rot = 30.4 ± 0.1 days, which translates to rotational velocity V rot = 19.5 ± 1.7 km s‑1. The s…

2024 The Astrophysical Journal
Gaia 1
Science Opportunities for IMAP-Lo Observations of Interstellar Neutral Hydrogen and Deuterium during a Maximum of Solar Activity
DOI: 10.3847/1538-4365/ad23e9 Bibcode: 2024ApJS..271...43K

Möbius, E.; Schwadron, N. A.; Bzowski, M. +1 more

Direct-sampling observations of interstellar neutral gas, including hydrogen and deuterium, have been performed for more than one cycle of solar activity by IBEX. The IBEX viewing is restricted to directions perpendicular to the spacecraft–Sun line, which limits the observations to several months each year. This restriction is removed in the forth…

2024 The Astrophysical Journal Supplement Series
Ulysses 1
Evidence of Third Dredge-up in Post-AGB Stars in Galactic Globular Clusters
DOI: 10.3847/1538-4357/ad0a89 Bibcode: 2024ApJ...961...24D

Dixon, William V.

To better understand the mixing and mass loss experienced by low-mass stars as they ascend the asymptotic giant branch (AGB), I have gathered from the literature the abundances of CNO and s-process elements in post-AGB stars in Galactic globular clusters. These species are mixed to the surface during third dredge-up (3DU) events, so their abundanc…

2024 The Astrophysical Journal
Gaia 1