Search Publications

Newly Discovered Wolf-Rayet Stars in M31
DOI: 10.3847/1538-3881/ace25f Bibcode: 2023AJ....166...68N

Massey, Philip; Neugent, Kathryn F.

The evolved massive star populations of the Local Group galaxies are generally thought to be well understood. However, recent work has suggested that the Wolf-Rayet (WR) content of M31 may have been underestimated. We therefore began a pilot project to search for new WRs in M31 and to reexamine the completeness of our previous WR survey, finished …

2023 The Astronomical Journal
Gaia 5
An inner warp discovered in the disk around HD 110058 using VLT/SPHERE and HST/STIS
DOI: 10.1051/0004-6361/202346720 Bibcode: 2023A&A...678A...8S

Ménard, F.; Milli, J.; Boccaletti, A. +16 more

Context. An edge-on debris disk was detected in 2015 around the young, nearby A0V star HD 110058. The disk showed features resembling those seen in the disk of β Pictoris that could indicate the presence of a perturbing planetary-mass companion in the system.
Aims: We investigated new and archival scattered light images of the disk in order t…

2023 Astronomy and Astrophysics
eHST 5
Detecting planetary mass companions near the water frost-line using JWST interferometry
DOI: 10.1093/mnras/stac3425 Bibcode: 2023MNRAS.519.2718R

Carter, Aarynn L.; Hinkley, Sasha; Sallum, Steph +4 more

JWST promises to be the most versatile infrared observatory for the next two decades. The Near Infrared and Slitless Spectrograph (NIRISS) instrument, when used in the Aperture Masking Interferometry (AMI) mode, will provide an unparalleled combination of angular resolution and sensitivity compared to any existing observatory at mid-infrared wavel…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 5
Determining satellite infall times using machine learning
DOI: 10.1093/mnras/stad222 Bibcode: 2023MNRAS.520.1704B

Cautun, Marius; Barmentloo, Stan

A key unknown of the Milky Way (MW) satellites is their orbital history, and, in particular, the time they were accreted onto the MW system since it marks the point where they experience a multitude of environmental processes. We present a new methodology for determining infall times, namely using a neural network (NN) algorithm. The NN is trained…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 5
Sulfur abundances in three Galactic clusters: Ruprecht 106, Trumpler 5, and Trumpler 20
DOI: 10.1051/0004-6361/202244646 Bibcode: 2023A&A...671A.137L

Bonifacio, P.; Caffau, E.; Monaco, L. +4 more

Context. Sulfur (S) is one of the lesser-studied α-elements. Published investigations of its behavior have so far focused on local stars, and only a few clusters of the Milky Way have been considered to study this topic. We aim to study the S content of the globular cluster Ruprecht 106 - which has never before been studied for this purpose, but i…

2023 Astronomy and Astrophysics
Gaia 5
Spectra of V1405 Cas at the Very Beginning Indicate a Low-mass ONeMg White Dwarf Progenitor
DOI: 10.3847/1538-4357/ad0133 Bibcode: 2023ApJ...958..156T

Maehara, Hiroyuki; Nogami, Daisaku; Yamanaka, Masayuki +9 more

The lowest possible mass of ONeMg white dwarfs (WDs) has not been clarified despite its importance in the formation and evolution of WDs. We tackle this issue by studying the properties of V1405 Cas (Nova Cassiopeiae 2021), which is an outlier given a combination of its very slow light-curve evolution and the recently reported neon-nova identifica…

2023 The Astrophysical Journal
Gaia 5
The blue supergiant Sher 25 revisited in the Gaia era
DOI: 10.1051/0004-6361/202347253 Bibcode: 2023A&A...677A.175W

Butler, K.; Weßmayer, D.; Przybilla, N. +2 more


Aims: The evolutionary status of the blue supergiant Sher 25 and its membership to the massive cluster NGC 3603 are investigated.
Methods: A hybrid non-local thermodynamic equilibrium (non-LTE) spectrum synthesis approach is employed to analyse a high-resolution optical spectrum of Sher 25 and five similar early B-type comparison stars i…

2023 Astronomy and Astrophysics
Gaia IUE 5
On the Migration Origin of the Hercules Moving Group with GAIA, LAMOST, APOGEE, and GALAH Surveys
DOI: 10.3847/1538-4357/acf295 Bibcode: 2023ApJ...956..146L

Wu, Yaqian; Zhao, Jingkun; Yoon, Suk-Jin +3 more

Using Gaia DR3 data and the wavelet transformation technique, we study the substructures of the Hercules moving group (HMG): Hercules 1 (H1) and Hercules 2 (H2). Spectroscopic survey data from LAMOST, APOGEE, and GALAH are used to obtain metallicities and ages of stars belonging to the HMG. Our analysis leads to several key findings as follows: (a…

2023 The Astrophysical Journal
Gaia 5
The effect of variations in the magnetic field direction from turbulence on kinetic-scale instabilities
DOI: 10.1051/0004-6361/202345965 Bibcode: 2023A&A...672L...4O

Verscharen, Daniel; Chen, Christopher H. K.; Opie, Simon +2 more

At kinetic scales in the solar wind, instabilities transfer energy from particles to fluctuations in the electromagnetic fields while restoring plasma conditions towards thermodynamic equilibrium. We investigate the interplay between background turbulent fluctuations at the small-scale end of the inertial range and kinetic instabilities acting to …

2023 Astronomy and Astrophysics
SolarOrbiter 5
The Influence of the Galactic Bar on the Dynamics of Globular Clusters
DOI: 10.3390/galaxies11010026 Bibcode: 2023Galax..11...26T

Carraro, Giovanni; Korchagin, Vladimir; Tkachenko, Roman +2 more

We make use of recent estimates for the parameters of the Milky Way's halo globular clusters and study the influence of the galactic bar on the dynamics of these clusters by computing their orbits. We use both an axisymmetric and non-axisymmetric galactic potentials, which include the rotating elongated bar/bulge structure. We account for observat…

2023 Galaxies
Gaia 5