Search Publications

JWST unveils the brown dwarf sequence of 47 Tucanæ
DOI: 10.1093/mnrasl/slad021 Bibcode: 2023MNRAS.521L..39N

Bedin, L. R.; Nardiello, D.; Griggio, M.

We have developed a technique to restore scientific usage in compromised (publicly available) images collected with the JWST of the Galactic globular cluster NGC 104 (47 Tucanæ). In spite of the degradation and limited data, we were able to recover photometry and astrometry for the coolest stellar objects ever observed within a globular cluster, p…

2023 Monthly Notices of the Royal Astronomical Society
Gaia eHST JWST 10
Investigating 16 Open Clusters in the Kepler/K2-Gaia DR3 Field. I. Membership, Binary Systems, and Rotation
DOI: 10.3847/1538-4365/ace5af Bibcode: 2023ApJS..268...30L

Bi, Shaolan; Ge, Zhishuai; Li, Tanda +9 more

Using data from Gaia Data Release 3 and Kepler/K2, we present a catalog of 16 open clusters with ages ranging from 4-4000 Myr that provides detailed information on membership, binary systems, and rotation. We assess the memberships in 5D phase space, and estimate the basic parameters of each cluster. Among the 20,160 members, there are 4381 stars …

2023 The Astrophysical Journal Supplement Series
Gaia 10
Red horizontal branch stars: An asteroseismic perspective
DOI: 10.1051/0004-6361/202245746 Bibcode: 2023A&A...671A..53M

Tailo, Marco; Stokholm, Amalie; Valentini, Marica +7 more

Robust age estimates of red giant stars are now possible thanks to the precise inference of their mass based on asteroseismic constraints. However, there are cases where such age estimates can be highly precise yet very inaccurate. An example is giants that have undergone mass loss or mass transfer events that have significantly altered their mass…

2023 Astronomy and Astrophysics
Gaia 10
Exploring the chemodynamics of metal-poor stellar populations
DOI: 10.1051/0004-6361/202347229 Bibcode: 2023A&A...677A..74D

Smiljanic, R.; da Silva, A. R.

Context. Metal-poor stars are key for studying the formation and evolution of the Galaxy. Evidence of the early mergers that built up the Galaxy remains in the distributions of abundances, kinematics, and orbital parameters of its stars. Several substructures resulting from these mergers have been tentatively identified in the literature.
Aim…

2023 Astronomy and Astrophysics
Gaia 10
Observing Atmospheric Escape in Sub-Jovian Worlds with JWST
DOI: 10.3847/1538-3881/accf10 Bibcode: 2023AJ....165..244D

Alam, Munazza K.; Espinoza, Néstor; Dos Santos, Leonardo A. +1 more

Hydrodynamic atmospheric escape is considered an important process that shapes the evolution of sub-Jovian exoplanets, particularly those with short orbital periods. The metastable He line in the near-infrared at 1.083 µm is a reliable tracer of atmospheric escape in hot exoplanets, with the advantage of being observable from the ground. How…

2023 The Astronomical Journal
JWST 10
Precise masses and ages of 1 million RGB and RC stars observed by LAMOST
DOI: 10.1051/0004-6361/202245809 Bibcode: 2023A&A...675A..26W

Huang, Yang; Zhang, Huawei; Wang, Chun +1 more

We construct a catalogue of stellar masses and ages for 696 680 red giant branch (RGB) stars, 180 436 primary red clump (RC) stars, and 120 907 secondary RC stars selected from the LAMOSTDR8. The RGBs, primary RCs, and secondary RCs are identified with the large frequency spacing (∆ν) and period spacing (∆P) estimated from the LAMOST spectra with …

2023 Astronomy and Astrophysics
Gaia 10
The outburst of the changing-look AGN IRAS 23226-3843 in 2019
DOI: 10.1051/0004-6361/202244786 Bibcode: 2023A&A...670A.103K

Schartel, N.; Komossa, S.; Kollatschny, W. +8 more


Aims: IRAS 23226-3843 has previously been classified as a changing-look active galactic nucleus (AGN) based on observations taken in the 1990s in comparison to X-ray data (Swift, XMM-Newton, and NuSTAR) and optical spectra taken after a very strong X-ray decline in 2017. In 2019, Swift observations revealed a strong rebrightening in X-ray and…

2023 Astronomy and Astrophysics
XMM-Newton 10
Water Vapor Vertical Distribution on Mars During Perihelion Season of MY 34 and MY 35 With ExoMars-TGO/NOMAD Observations
DOI: 10.1029/2022JE007273 Bibcode: 2023JGRE..12807273B

Aoki, S.; Vandaele, A. C.; Daerden, F. +18 more

The water vapor in the Martian atmosphere plays a significant role in the planet's climate, being crucial in most of the chemical and radiative transfer processes. Despite its importance, the vertical distribution of H2O in the atmosphere has not still been characterized precisely enough. The recent ExoMars Trace Gas Orbiter mission, wi…

2023 Journal of Geophysical Research (Planets)
ExoMars-16 10
Backstreaming ions at a high Mach number interplanetary shock. Solar Orbiter measurements during the nominal mission phase
DOI: 10.1051/0004-6361/202347006 Bibcode: 2023A&A...679A.106D

Vainio, R.; Owen, C. J.; Wimmer-Schweingruber, R. F. +9 more

Context. Solar Orbiter, a mission developed by the European Space Agency, explores in situ plasma across the inner heliosphere while providing remote-sensing observations of the Sun. The mission aims to study the solar wind, but also transient structures such as interplanetary coronal mass ejections and stream interaction regions. These structures…

2023 Astronomy and Astrophysics
SolarOrbiter 10
Surface structure of 45 Hercules: an otherwise unremarkable Ap star with a surprisingly weak magnetic field
DOI: 10.1093/mnras/stad720 Bibcode: 2023MNRAS.521.3480K

Petit, P.; Amarsi, A. M.; Kochukhov, O. +3 more

The origin of magnetic fields and their role in chemical spot formation on magnetic Ap stars is currently not understood. Here, we contribute to solving this problem with a detailed observational characterization of the surface structure of 45 Her, a weak-field Ap star. We find this object to be a long-period, single-lined spectroscopic binary and…

2023 Monthly Notices of the Royal Astronomical Society
Gaia 10