Search Publications

A meeting at z ∼ 3: Young massive galaxies and an AGN within 30 kpc of the luminous QSO LBQS 0302-0019
DOI: 10.1051/0004-6361/202140898 Bibcode: 2021A&A...653A.122H

Sander, A. A. C.; Shanks, T.; Husemann, B. +2 more

Context. Contrary to expectations from scenarios of black hole growth driven by galaxy interactions and mergers, dual active galactic nuclei (AGN) with kiloparsec separations are rarely observed and are very difficult to identify, in particular at high redshifts (i.e. z > 2).
Aims: Focussing on the recently discovered dual AGN system LBQS …

2021 Astronomy and Astrophysics
eHST 3
LIStEN: L' band Imaging Survey for Exoplanets in the North
DOI: 10.1051/0004-6361/202039541 Bibcode: 2021A&A...645A..88M

Henning, Thomas; Ertel, Steve; Musso Barcucci, Arianna +9 more

Context. Planetary systems and debris discs are natural by-products of the star formation process, and they affect each other. The direct imaging technique allows simultaneous imaging of both a companion and the circumstellar disc it resides in, and is thus a valuable tool to study companion-disc interactions. However, the number of systems in whi…

2021 Astronomy and Astrophysics
Gaia Herschel 3
Heavy-element Rydberg transition line emission from the post-giant-evolution star HD 101584
DOI: 10.1051/0004-6361/202140537 Bibcode: 2021A&A...651A..35O

Lindqvist, M.; Olofsson, H.; Black, J. H. +7 more

Context. We report the detection of two lines at millimetre wavelengths towards the immediate surroundings of the post-giant and most likely post-common-envelope star HD 101584 using high-angular-resolution ALMA observations. The circumstellar environment of this object is rich in different molecular species, but we find no viable identifications …

2021 Astronomy and Astrophysics
Gaia 3
Orbital eccentricities as indicators of stellar populations. A kinematical analysis of the local disc from Gaia DR2 catalogue
DOI: 10.1051/0004-6361/202040017 Bibcode: 2021A&A...649A..48C

Cubarsi, R.; Stojanović, M.; Ninković, S.


Aims: Based on a local sample from Gaia DR2 catalogue composed of 74 339 stars, we are able to derive more accurate kinematic statistics defining the local stellar populations and classify the stars in terms of their planar and vertical orbital eccentricities.
Methods: Firstly, we carried out a kinematical characterisation of stellar pop…

2021 Astronomy and Astrophysics
Gaia 3
Magnetic flux structuring of the quiet Sun internetwork. Center-to-limb analysis of solar-cycle variations
DOI: 10.1051/0004-6361/202140705 Bibcode: 2021A&A...651A..21F

Faurobert, M.; Ricort, G.

Context. The small-scale magnetism of the quiet Sun has been investigated by various means in recent decades. It is now well established that the quiet Sun contains in total more magnetic flux than active regions and represents an important reservoir of magnetic energy. But the nature and evolution of these fields remain largely unknown.
Aims…

2021 Astronomy and Astrophysics
Hinode 2
Systematic search for lensed X-ray sources in the CLASH fields
DOI: 10.1051/0004-6361/202040249 Bibcode: 2021A&A...648A..47L

Nonino, Mario; Grillo, Claudio; Rosati, Piero +8 more


Aims: We exploit the high angular resolution of Chandra to search for unresolved X-ray emission from lensed sources in the field of view of 11 CLASH clusters, whose critical lines and amplification maps were previously obtained with accurate strong-lensing models. We consider a solid angle in the lens plane corresponding to a magnification &m…

2021 Astronomy and Astrophysics
eHST 2
Properties of the brightest globular cluster in M 81 based on multicolour observations
DOI: 10.1051/0004-6361/202140574 Bibcode: 2021A&A...649A.138W

Ma, Jun; Wang, Shoucheng

Context. Researching the properties of the brightest globular cluster (referred to as GC1) in M 81 can provide a fossil record of the earliest stages of galaxy formation and evolution. The Beijing-Arizona-Taiwan-Connecticut (BATC) Multicolour Sky Survey has carried out deep exposures of M 81.
Aims: We derive the magnitudes in intermediate-ban…

2021 Astronomy and Astrophysics
eHST 2
Nonsequential neural network for simultaneous, consistent classification, and photometric redshifts of OTELO galaxies
DOI: 10.1051/0004-6361/202141360 Bibcode: 2021A&A...655A..56D

Cepa, J.; Pérez García, A. M.; Alfaro, E. J. +17 more

Context. Computational techniques are essential for mining large databases produced in modern surveys with value-added products.
Aims: This paper presents a machine learning procedure to carry out a galaxy morphological classification and photometric redshift estimates simultaneously. Currently, only a spectral energy distribution (SED) fitti…

2021 Astronomy and Astrophysics
eHST 2
Evidence for local particle acceleration in the first recurrent galactic cosmic ray depression observed by Solar Orbiter. The ion event on 19 June 2020
DOI: 10.1051/0004-6361/202140966 Bibcode: 2021A&A...656L..10A

Fedorov, A.; Kulkarni, S. R.; Lario, D. +61 more

Context. In mid-June 2020, the Solar Orbiter (SolO) mission reached its first perihelion at 0.51 au and started its cruise phase, with most of the in situ instruments operating continuously.
Aims: We present the in situ particle measurements of the first proton event observed after the first perihelion obtained by the Energetic Particle Detec…

2021 Astronomy and Astrophysics
SolarOrbiter 2
Orbital and sub-orbital period determination of the candidate high-mass X-ray binary HD 3191
DOI: 10.1051/0004-6361/202140545 Bibcode: 2021A&A...651A...1M

Luque-Escamilla, Pedro L.; Martí, Josep; Paredes, Josep M. +1 more


Aims: The final aim of this paper is to expand the sparse group of X-ray binaries with gamma-ray counterparts as laboratories to study high-energy processes under physical conditions that periodically repeat.
Methods: A follow-up of a candidate system has been carried out. We applied both photometric and spectroscopic techniques in the o…

2021 Astronomy and Astrophysics
Gaia 2