Search Publications

The truncation of the disk of NGC 4565. Detected up to z = 4 kpc, with star formation, and affected by the warp
DOI: 10.1051/0004-6361/202346280 Bibcode: 2023A&A...678A..62M

Trujillo, Ignacio; Borlaff, Alejandro S.; Comerón, Sébastien +5 more

Context. The hierarchical model of galaxy formation suggests that galaxies are continuously growing. However, our position inside the Milky Way prevents us from studying the disk edge. Truncations are low surface brightness features located in the disk outskirts of external galaxies. They indicate where the disk brightness abruptly drops, and thei…

2023 Astronomy and Astrophysics
Gaia 4
A rotational age for the open cluster NGC 2281. The possibility of using the fast rotator sequence for accurate cluster age determinations
DOI: 10.1051/0004-6361/202346083 Bibcode: 2023A&A...674A.152F

Strassmeier, K. G.; Granzer, T.; Barnes, S. A. +3 more

Context. Cool star rotation periods have become an important tool in determining ages of open clusters.
Aims: We aim to estimate the age of the open cluster NGC 2281 based on the rotational properties of its low-mass members. Previous age estimates for this open cluster range from 275 Myr to 630 Myr.
Methods: Based on an eight month-long…

2023 Astronomy and Astrophysics
Gaia 4
Radio multiwavelength analysis of the compact disk CX Tau: Presence of strong free-free variability or anomalous microwave emission
DOI: 10.1051/0004-6361/202347042 Bibcode: 2023A&A...677A.118C

Lodato, G.; Testi, L.; Tazzari, M. +8 more

Protoplanetary disks emit radiation across a broad range of wavelengths, requiring a multiwavelength approach to fully understand their physical mechanisms and how they form planets. Observations at submillimeter to centimeter wavelengths can provide insights into the thermal emission from dust, free-free emission from ionized gas, and possible gy…

2023 Astronomy and Astrophysics
Gaia 4
The multichord stellar occultation by the centaur Bienor on January 11, 2019
DOI: 10.1051/0004-6361/202243214 Bibcode: 2023A&A...669A.112F

Colas, F.; Mottola, S.; Souami, D. +42 more

Within our program of physical characterization of trans-Neptunian objects and centaurs, we predicted a stellar occultation by the centaur (54598) Bienor to occur on January 11, 2019, with good observability potential. We obtained high accuracy astrometric data to refine the prediction, resulting in a shadow path favorable for the Iberian Peninsul…

2023 Astronomy and Astrophysics
Gaia 4
Dynamical state of the globular clusters Rup 106 and IC 4499
DOI: 10.1051/0004-6361/202244288 Bibcode: 2023A&A...670A..11B

Dalessandro, E.; Beccari, G.; Cadelano, M.

The dynamical evolution of globular clusters is theoretically described by a series of well-known events typical of N-body systems. Still, the identification of observational signatures able to empirically describe the stage of dynamical evolution of a stellar system with a density typical of a globular cluster represents a challenge. In this pape…

2023 Astronomy and Astrophysics
Gaia eHST 4
Temperature diagnostics of chromospheric fibrils
DOI: 10.1051/0004-6361/202245527 Bibcode: 2023A&A...672A..89K

Oliver, R.; Kuridze, D.; Kriginsky, M.

Context. Chromospheric fibrils are thin and elongated structures that connect nearby photospheric magnetic field concentrations of opposite polarities.
Aims: We assess the possibilities and drawbacks related to the use of current instrumentation and inversion techniques to infer the thermodynamic structure of chromospheric fibrils.
Metho…

2023 Astronomy and Astrophysics
IRIS 4
Mining archival data from wide-field astronomical surveys in search of near-Earth objects
DOI: 10.1051/0004-6361/202345957 Bibcode: 2023A&A...673A..93S

Koschny, Detlef; Verdoes Kleijn, Gijs; Micheli, Marco +5 more

Context. Increasing our knowledge of the orbits and compositions of near-earth objects (NEOs) is important for a better understanding of the evolution of the Solar System and life. The detection of serendipitous NEO appearances among the millions of archived exposures from large astronomical imaging surveys can provide a contribution which is comp…

2023 Astronomy and Astrophysics
Gaia 4
Finding the dispersing siblings of young open clusters. Dynamical traceback simulations using Gaia DR3
DOI: 10.1051/0004-6361/202346877 Bibcode: 2023A&A...679A.105V

Prusti, T.; Hobbs, D.; McMillan, P. +1 more

Context. Stars tend to form in clusters, but many escape their birth clusters very early. Identifying the escaped members of clusters can inform us about the dissolution of star clusters, but also about the stellar dynamics in the galaxy. Methods capable of finding escaped stars from many clusters are required to fully exploit the large amounts of…

2023 Astronomy and Astrophysics
Gaia 4
VPNEP: Detailed characterization of TESS targets around the Northern Ecliptic Pole. I. Survey design, pilot analysis, and initial data release
DOI: 10.1051/0004-6361/202245255 Bibcode: 2023A&A...671A...7S

Strassmeier, K. G.; Weber, M.; Gruner, D. +13 more

Context. We embarked on a high-resolution optical spectroscopic survey of bright Transiting Exoplanet Survey Satellite (TESS) stars around the Northern Ecliptic Pole (NEP), dubbed the Vatican-Potsdam-NEP (VPNEP) survey.
Aims: Our NEP coverage comprises ≈770 square degrees with 1067 stars, of which 352 are bona fide dwarf stars and 715 are gia…

2023 Astronomy and Astrophysics
Gaia 4
Constraints on the non-thermal desorption of methanol in the cold core LDN 429-C
DOI: 10.1051/0004-6361/202245157 Bibcode: 2023A&A...670A.141T

Boogert, A. C. A.; Gratier, P.; Dartois, E. +6 more

Context. Cold cores are one of the first steps of star formation, characterized by densities of a few 104-105 cm−3, low temperatures (15 K and below), and very low external UV radiation. In these dense environments, a rich chemistry takes place on the surfaces of dust grains. Understanding the physico-chemical proc…

2023 Astronomy and Astrophysics
Herschel 4