Search Publications

The bright blue side of the night sky: Spectroscopic survey of bright and hot (pre-) white dwarfs
DOI: 10.1051/0004-6361/202346865 Bibcode: 2023A&A...677A..29R

Kepler, S. O.; Uzundag, Murat; Pelisoli, Ingrid +10 more

We report on the spectroscopic confirmation of 68 new bright (G = 13.5-17.2 mag) and blue (pre-)white dwarfs (WDs). This finding has allowed us to almost double the number of the hottest (Teff ≥ 60 kK) known WDs brighter than G = 16 mag. We increased the number of known ultra-high excitation (UHE) WDs by 20%, found one unambiguous close…

2023 Astronomy and Astrophysics
Gaia 12
A radio-jet-driven outflow in the Seyfert 2 galaxy NGC 2110?
DOI: 10.1051/0004-6361/202245408 Bibcode: 2023A&A...675A..58P

Rigopoulou, D.; Hönig, S. F.; Villar-Martín, M. +16 more

We present a spatially resolved study of the ionized gas in the central 2 kpc of the Seyfert 2 galaxy NGC 2110 and investigate the role of its moderate-luminosity radio jet (kinetic radio power of Pjet = 2.3 × 1043 erg s−1). We used new optical integral-field observations taken with the MEGARA spectrograph at the G…

2023 Astronomy and Astrophysics
Gaia eHST 12
The young massive SMC cluster NGC 330 seen by MUSE. III. Stellar parameters and rotational velocities
DOI: 10.1051/0004-6361/202345950 Bibcode: 2023A&A...680A..32B

Wang, C.; Dufton, P. L.; de Mink, S. E. +11 more

Context. The origin of the initial rotation rates of stars, and how a star's surface rotational velocity changes during the evolution, either by internal angular momentum transport or due to interactions with a binary companion, remain open questions in stellar astrophysics.
Aims: Here, we aim to derive the physical parameters and study the d…

2023 Astronomy and Astrophysics
eHST 12
Hydrogen column density variability in a sample of local Compton-thin AGN
DOI: 10.1051/0004-6361/202345947 Bibcode: 2023A&A...678A.154T

Ajello, M.; Marchesi, S.; Torres-Albà, N. +5 more

We present the analysis of multiepoch observations of a set of 12 variable, Compton-thin, local (z < 0.1) active galactic nuclei (AGN) selected from the 100-month BAT catalog. We analyzed all available X-ray data from Chandra, XMM-Newton, and NuSTAR, adding up to a total of 53 individual observations. This corresponds to between three and seven…

2023 Astronomy and Astrophysics
XMM-Newton 12
Photometric variability of the LAMOST sample of magnetic chemically peculiar stars as seen by TESS
DOI: 10.1051/0004-6361/202346657 Bibcode: 2023A&A...676A..55L

Paunzen, E.; Shultz, M. E.; Bernhard, K. +2 more

Context. High-quality light curves from space-based missions have opened up a new window on the rotational and pulsational properties of magnetic chemically peculiar (mCP) stars and have fuelled asteroseismic studies. They allow the internal effects of surface magnetic fields to be probed and numerous astrophysical parameters to be derived with gr…

2023 Astronomy and Astrophysics
Gaia 12
Evolution of the Lyman-α-emitting fraction and UV properties of lensed star-forming galaxies in the range 2.9 < z < 6.7
DOI: 10.1051/0004-6361/202347110 Bibcode: 2023A&A...678A.174G

Richard, J.; Pello, R.; Tuan-Anh, P. +6 more

Context. Faint galaxies are theorised to have played a major role, perhaps the dominant role, in reionising the Universe. Their properties, as well as the Lyman-α emitter (LAE) fraction, XLAE, could provide useful insights into this epoch.
Aims: We used four clusters of galaxies from the Lensed Lyman-alpha MUSE Arcs Sample (LLAMAS)…

2023 Astronomy and Astrophysics
eHST 12
Forbidden hugs in pandemic times. IV. Panchromatic evolution of three luminous red novae
DOI: 10.1051/0004-6361/202244684 Bibcode: 2023A&A...671A.158P

Fugazza, D.; Lundqvist, P.; Reichart, D. E. +77 more

We present photometric and spectroscopic data on three extragalactic luminous red novae (LRNe): AT 2018bwo, AT 2021afy, and AT 2021blu. AT 2018bwo was discovered in NGC 45 (at about 6.8 Mpc) a few weeks after the outburst onset. During the monitoring per…

2023 Astronomy and Astrophysics
eHST 12
The high-albedo, low polarization disk around HD 114082 that harbors a Jupiter-sized transiting planet. Constraints from VLT/SPHERE completed with TESS, Gaia, and radial velocities
DOI: 10.1051/0004-6361/202244380 Bibcode: 2023A&A...672A...1E

Ménard, F.; Marshall, J. P.; del Burgo, C. +36 more


Aims: We present new optical and near-infrared images of the debris disk around the F-type star HD 114082 in the Scorpius-Centaurus OB association. We obtained direct imaging observations and analyzed the TESS photometric time series data of this target with the goal of searching for planetary companions to HD 114082 and characterizing the mo…

2023 Astronomy and Astrophysics
Gaia 12
Detection of open cluster rotation fields from Gaia EDR3 proper motions
DOI: 10.1051/0004-6361/202142826 Bibcode: 2023A&A...673A.128G

Krone-Martins, A.; Moitinho, A.; Guilherme-Garcia, P.

Context. Most stars from in groups which with time disperse, building the field population of their host galaxy. In the Milky Way, open clusters have been continuously forming in the disk up to the present time, providing it with stars spanning a broad range of ages and masses. Observations of the details of cluster dissolution are, however, scarc…

2023 Astronomy and Astrophysics
Gaia 12
Identifying the energy release site in a solar microflare with a jet
DOI: 10.1051/0004-6361/202244996 Bibcode: 2023A&A...670A..56B

Monstein, Christian; Krucker, Säm; Veronig, Astrid M. +10 more

Context. One of the main science questions of the Solar Orbiter and Parker Solar Probe missions deals with understanding how electrons in the lower solar corona are accelerated and how they subsequently access interplanetary space.
Aims: We aim to investigate the electron acceleration and energy release sites as well as the manner in which ac…

2023 Astronomy and Astrophysics
SolarOrbiter 12