Search Publications

The ALPINE-ALMA [CII] survey: Dust emission effective radius up to 3 kpc in the early Universe
DOI: 10.1051/0004-6361/202348996 Bibcode: 2024A&A...686A.187P

Cimatti, A.; Pozzi, F.; Magdis, G. E. +25 more


Aims: Measurements of the size of dust continuum emission are an important tool for constraining the spatial extent of star formation, and hence the buildup of stellar mass. Compact dust emission has generally been observed at cosmic noon (z ∼ 2 − 3). However, at earlier epochs, toward the end of the reionization (z ∼ 4 − 6), only the sizes o…

2024 Astronomy and Astrophysics
eHST 9
Modeling the propagation of coronal mass ejections with COCONUT: Implementation of the regularized Biot-Savart law flux rope model
DOI: 10.1051/0004-6361/202347634 Bibcode: 2024A&A...683A..54G

Schmieder, B.; Poedts, S.; Guo, Y. +8 more

Context. Coronal mass ejections (CMEs) are rapid eruptions of magnetized plasma that occur on the Sun. They are known to be the main drivers of adverse space weather. The accurate tracking of their evolution in the heliosphere in numerical models is of the utmost importance for space weather forecasting.
Aims: The main objective of this paper…

2024 Astronomy and Astrophysics
Hinode 9
Improving metallicity estimates for very metal-poor stars in the Gaia DR3 GSP-Spec catalog
DOI: 10.1051/0004-6361/202245762 Bibcode: 2024A&A...685A..59M

Helmi, Amina; Matsuno, Tadafumi; Starkenburg, Else +1 more

Context. In the latest Gaia Data Release (DR3), the GSP-Spec module has provided stellar parameters and chemical abundances measured from the RVS spectra alone. However, the GSP-Spec parameters - including metallicity - for very metal-poor (VMP; [Fe/H] < −2) stars suffer from parameter degeneracy due to a lack of information in their spectra, a…

2024 Astronomy and Astrophysics
Gaia 8
Discovery of a > 13 Mpc long X-ray filament between two galaxy clusters beyond three times their virial radii
DOI: 10.1051/0004-6361/202449354 Bibcode: 2024A&A...691A.286D

Pacaud, F.; Reiprich, T. H.; Dolag, K. +5 more

Context. A significant fraction of the missing baryons in the local Universe is expected to reside in large-scale filaments that may be observable in soft X-ray emission. Until now, however, very few candidate emission filaments have been found in individual systems, and none beyond three times the virial radius of the clusters at the nodes of the…

2024 Astronomy and Astrophysics
XMM-Newton 8
The structural properties of multiple populations in globular clusters: The instructive case of NGC 3201
DOI: 10.1051/0004-6361/202349021 Bibcode: 2024A&A...685A.158C

Vesperini, Enrico; Cadelano, Mario; Dalessandro, Emanuele

All multiple population (MP) formation models in globular clusters (GCs) predict that second population (SP) stars form more centrally concentrated than the first population (FP). As dynamical evolution proceeds, spatial differences are progressively erased and only dynamically young clusters are expected to retain a partial memory of the initial …

2024 Astronomy and Astrophysics
Gaia eHST 8
The MEGARA view of outflows in LINERs
DOI: 10.1051/0004-6361/202347675 Bibcode: 2024A&A...683A..43H

Hermosa Muñoz, L.; Márquez, I.; Masegosa, J. +12 more

Context. Feedback processes, in particular those driven by outflows, are believed to play a major role in galaxy evolution. Outflows are believed to be ubiquitous in all active galactic nuclei (AGNs), although their presence in low luminosity AGNs, in particular for Low-Ionisation Nuclear Emission line Regions (LINERs), has only started to be expl…

2024 Astronomy and Astrophysics
eHST 8
Eclipse-timing study of new hierarchical triple star candidates in the northern continuous viewing zone of TESS
DOI: 10.1051/0004-6361/202348909 Bibcode: 2024A&A...685A..43M

Mitnyan, T.; Pál, A.; Borkovits, T. +4 more


Aims: We compiled a list of more than 3500 eclipsing binaries located in and near the northern continuous viewing zone (NCVZ) of the TESS space telescope that have sufficient TESS photometry to search for additional hidden components in these systems. In addition to discovering their hierarchical nature, we also determined their orbital param…

2024 Astronomy and Astrophysics
Gaia 8
The multi-spacecraft high-energy solar particle event of 28 October 2021
DOI: 10.1051/0004-6361/202346045 Bibcode: 2024A&A...682A.106K

Vainio, R.; Rodríguez-Pacheco, J.; Wimmer-Schweingruber, R. F. +15 more


Aims: We studied the first multi-spacecraft high-energy solar energetic particle (SEP) event of solar cycle 25, which triggered a ground level enhancement on 28 October 2021, using data from multiple observers (Parker Solar Probe, STEREO-A, Solar Orbiter, GOES, SOHO, BepiColombo, and the Mars Science Laboratory) that were widely distributed t…

2024 Astronomy and Astrophysics
SOHO SolarOrbiter 8
Low-redshift Lyman Continuum Survey (LzLCS). Radio continuum properties of low-z Lyman continuum emitters
DOI: 10.1051/0004-6361/202348416 Bibcode: 2024A&A...688A.198B

Pentericci, Laura; Jaskot, Anne E.; Flury, Sophia R. +20 more

Context. Sources that leak Lyman continuum (LyC) photons and lead to the reionisation of the universe are an object of intense study using multiple observing facilities. Recently, the Low-redshift LyC Survey (LzLCS) has presented the first large sample of LyC emitting galaxies at low redshift (z ∼ 0.3) with the Hubble Space Telescope Cosmic Origin…

2024 Astronomy and Astrophysics
eHST 8
Forming localized dust concentrations in a dust ring: DM Tau case study. The asymmetric 7 mm dust continuum of the DM Tau disk
DOI: 10.1051/0004-6361/202348896 Bibcode: 2024A&A...685A..18L

Dong, Ruobing; Kataoka, Akimasa; Liu, Hauyu Baobab +8 more

Context. Previous high-angular-resolution 225 GHz (~1.3 mm) continuum observations of the transitional disk DM Tau have resolved an outer ring at 20-120 au radii that is weakly azimuthally asymmetric.
Aims: We aim to examine dust growth and filtration in the outer ring of DM Tau.
Methods: We performed ~0″.06 (~8.7 au) resolution Karl G. …

2024 Astronomy and Astrophysics
Gaia 8