Search Publications

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
Col-OSSOS: The Two Types of Kuiper Belt Surfaces
DOI: 10.3847/PSJ/acc844 Bibcode: 2023PSJ.....4...80F

Marsset, Michaël; Fraser, Wesley C.; Pike, Rosemary E. +12 more

The Colors of the Outer Solar System Origins Survey (Col-OSSOS) has gathered a high-quality, near-simultaneous, and brightness-complete sample of (g - r) and (r - J) colors for 102 Kuiper Belt objects (KBOs) with (u - g) and (r - z) gathered for some. We present the current state of the survey and data analysis. Recognizing that the optical colors…

2023 The Planetary Science Journal
eHST 10
Dust Properties of 870 µm-selected Galaxies in GOODS-S
DOI: 10.3847/1538-4357/acd1e5 Bibcode: 2023ApJ...951...48M

Bauer, F. E.; Barger, A. J.; Cowie, L. L. +2 more

We analyze the dust properties of 57 870 µm-selected dusty star-forming galaxies in GOODS-S using new deep Atacama Large Millimeter/Submillimeter Array 1.2, 2, and 3 mm continuum imaging together with other far-infrared through millimeter data. We fit the spectral energy distributions (SEDs) with optically thin modified blackbodies to constr…

2023 The Astrophysical Journal
Herschel 10
Combining HIPPARCOS and Gaia data for the study of binaries: The BINARYS tool
DOI: 10.1051/0004-6361/202244144 Bibcode: 2023A&A...672A..82L

Arenou, F.; Babusiaux, C.; van Leeuwen, F. +6 more

Context. Orbital motion in binary and planetary systems is the main source of precise stellar and planetary mass measurements, and the joint analysis of data obtained using multiple observational methods can both lift degeneracies and improve precision.
Aims: We set out to measure the masses of individual stars in binary systems using all the…

2023 Astronomy and Astrophysics
Gaia Hipparcos 10