Search Publications

The Lockman-SpReSO project. Galactic flows in a sample of far-infrared galaxies
DOI: 10.1051/0004-6361/202347826 Bibcode: 2024A&A...684A..31G

Krongold, Yair; Gallego, Jesús; Sánchez-Portal, Miguel +21 more

Context. The Lockman-SpReSO project is an optical spectroscopic survey of 956 far-infrared (FIR) objects within the Lockman Hole field limited by magnitude RC(AB) < 24.5. Fe II and Mg II absorption lines have been detected in 21 out of 456 objects with a determined spectroscopic redshift in the catalogue. The redshifts of these objec…

2024 Astronomy and Astrophysics
eHST 0
Spectral aging analysis of the 3C 219 double-double radio galaxy
DOI: 10.1051/0004-6361/202450897 Bibcode: 2024A&A...691A..76W

Jamrozy, M.; Wolnik, K.; Jurusik, W.

Context. Double-double radio galaxies are characterized by intermittent jet-formation activity. The exact reasons for this behavior are not yet fully understood. Studying these objects and their environment allows us to find common characteristics and compare them with the general population of radio galaxies. 3C 219 is a well-known and thoroughly…

2024 Astronomy and Astrophysics
eHST 0
A new sample of super-slowly rotating Ap (ssrAp) stars from the Zwicky Transient Facility survey
DOI: 10.1051/0004-6361/202452075 Bibcode: 2024A&A...692A.231H

Paunzen, E.; Bernhard, K.; Hümmerich, S.

Context. The magnetic chemically peculiar Ap stars exhibit an extreme spread of rotational velocities, the cause of which is not clearly understood. Ap stars with rotation periods of 50 days or longer are know as super-slowly rotating Ap (ssrAp) stars. Photometrically variable Ap stars are commonly termed α2 Canum Venaticorum (ACV) vari…

2024 Astronomy and Astrophysics
Gaia 0
Direct imaging and dynamical mass of a benchmark T-type brown dwarf companion to HD 167665
DOI: 10.1051/0004-6361/202451184 Bibcode: 2024A&A...691A.263M

Lutz, D.; Genzel, R.; Sturm, E. +111 more

Context. A low-mass companion potentially in the brown dwarf mass regime was discovered on a ~12 yr orbit (~5.5 au) around HD 167665 using radial velocity (RV) monitoring. Joint RV–astrometry analyses confirmed that HD 167665B is a brown dwarf with precisions on the measured mass of ~4–9%. Brown dwarf companions with measured mass and luminosity a…

2024 Astronomy and Astrophysics
Gaia Hipparcos 0
S-process nucleosynthesis in chemically peculiar binaries
DOI: 10.1051/0004-6361/202450299 Bibcode: 2024A&A...691A.128D

Hansen, C. J.; Kubátová, B.; Stateva, I. +4 more

Context. Around half of the heavy elements in the Universe are formed through the slow neutron capture (s-) process, which takes place in thermally pulsing asymptotic giant branch (AGB) stars with masses of 1 ‑ 6 M. The nucleosynthetic imprint of the s-process can be studied by observing the material on the surface of binary barium (Ba…

2024 Astronomy and Astrophysics
Gaia 0
Dissecting the planetary nebula NGC 4361 with MUSE
DOI: 10.1051/0004-6361/202449950 Bibcode: 2024A&A...690A.264W

Walsh, J. R.; Monreal Ibero, A.; Laging, J. +1 more

Context. Optical integral field spectroscopy of planetary nebulae (PNe) offers a unique tool to explore the spatial relationships between the complex mixture of the many components (neutral, low- and high-ionisation gas, dust, and the central star) and their underlying physical conditions. Aims. The optical line and continuum emission in the very-…

2024 Astronomy and Astrophysics
Gaia 0
Measuring the diffuse interstellar bands at 5780, 5797, and 6614 Å in low-resolution spectra of cool stars from LAMOST
DOI: 10.1051/0004-6361/202451408 Bibcode: 2024A&A...691A.282M

Jiang, Bi-Wei; Luo, A. -Li; Zhao, He +7 more

Context. The limited number of high-resolution spectra of hot stars is inadequate for statistical studies of diffuse interstellar bands (DIBs). In contrast, the vast quantity of low-resolution spectroscopic surveys on cool stars holds great potential for investigating the relationship between DIBs and the known interstellar medium (ISM), as well a…

2024 Astronomy and Astrophysics
Gaia 0
Resolved properties of a luminous hinge clump in the compact group of galaxies NGC 6845
DOI: 10.1051/0004-6361/202348869 Bibcode: 2024A&A...687A..33O

Torres-Flores, Sergio; Firpo, Veronica; Mora, Marcelo D. +2 more

Context. Compact groups of galaxies are unique places where galaxy-galaxy interactions play a mayor role on the evolution of its members. These strong gravitational encounters can induce star formation bursts.
Aims: We study the properties of one of the most luminous so-called hinge clumps that is located in the compact group of galaxies NGC …

2024 Astronomy and Astrophysics
eHST 0
Abnormal Stokes V profiles observed by Hinode in a sunspot: Detection of hidden photospheric fine-structures
DOI: 10.1051/0004-6361/202450625 Bibcode: 2024A&A...691A.274H

Rezaei, R.; Hamedivafa, H.

Context. Hidden magnetic components in a sunspot are present as small-scale structures that are absent in low-resolution observations. Aims. We search for traces of the hidden magnetic components in spectro-polarimetric observations of a mature sunspot close to the disk center recorded by Hinode. Methods. To find extra humps in the far blue and re…

2024 Astronomy and Astrophysics
Hinode 0
The return of FarNet-II: Generation of solar far-side magnetograms from helioseismic data
DOI: 10.1051/0004-6361/202451625 Bibcode: 2024A&A...692A.182B

Asensio Ramos, A.; Felipe, T.; Broock, E. G.

Context. The far-side activity of the Sun can be inferred by interpreting the near-side wave field using local helioseismic techniques. However, detections are limited to strongly active regions because signal-to-noise ratio of the data is low. Recently, we developed the FarNet and FarNet-II neural networks to improve the identification of active …

2024 Astronomy and Astrophysics
SolarOrbiter 0