Search Publications

SN 2021adxl: A luminous nearby interacting supernova in an extremely low-metallicity environment
DOI: 10.1051/0004-6361/202349036 Bibcode: 2024A&A...690A.259B

Drake, A. J.; Sollerman, J.; Fransson, C. +17 more

SN 2021adxl is a slowly evolving, luminous, Type IIn supernova with asymmetric emission line profiles, similar to the well-studied SN 2010jl. We present extensive optical, near-ultraviolet, and near-infrared photometry and spectroscopy covering ∼1.5 years post discovery. SN 2021adxl occurred in an unusual environment, atop a vigorously star-formin…

2024 Astronomy and Astrophysics
eHST 13
X-Shooting ULLYSES: Massive stars at low metallicity. II. DR1: Advanced optical data products for the Magellanic Clouds
DOI: 10.1051/0004-6361/202347479 Bibcode: 2024A&A...688A.104S

Hamann, W. -R.; Blomme, R.; Mehner, A. +34 more

Context. The XShootU project aims to obtain ground-based optical to near-infrared spectroscopy of all targets observed by the Hubble Space Telescope (HST) under the Director's Discretionary program ULLYSES. Using the medium-resolution spectrograph X-shooter, spectra of 235 OB and Wolf-Rayet (WR) stars in subsolar metallicity environments have been…

2024 Astronomy and Astrophysics
eHST 13
A census of new globular clusters in the Galactic bulge
DOI: 10.1051/0004-6361/202346377 Bibcode: 2024A&A...687A.201B

Bica, E.; Barbuy, B.; Ortolani, S. +1 more

Context. The number of known globular clusters in the Galactic bulge has been increasing steadily thanks to different new surveys. Aims. The aim of this study is to provide a census of the newly revealed globular clusters in the Galactic bulge, and analyze their characteristics. Methods. In recent years, many globular clusters have been discovered…

2024 Astronomy and Astrophysics
Gaia eHST 13
JWST discovers an AGN ionization cone but only weak radiatively driven feedback in a powerful z ≈ 3.5 radio-loud AGN
DOI: 10.1051/0004-6361/202348531 Bibcode: 2024A&A...683A.169W

Lehnert, Matthew D.; Zakamska, Nadia L.; Stern, Daniel +7 more

We present the first results from a JWST program studying the role played by powerful radio jets in the evolution of the most massive galaxies at the onset of cosmic noon. Using NIRSpec integral field spectroscopy, we detected 24 rest-frame optical emission lines from the z = 3.5892 radio galaxy 4C+19.71, which contains one of the most energetic r…

2024 Astronomy and Astrophysics
Gaia eHST JWST 13
The Galactic bulge exploration. I. The period-absolute magnitude-metallicity relations for RR Lyrae stars for GBP, V, G, GRP, I, J, H, and Ks passbands using Gaia DR3 parallaxes
DOI: 10.1051/0004-6361/202347338 Bibcode: 2024A&A...684A.176P

Prudil, Z.; Kunder, A.; Koch-Hansen, A. J. +1 more

We present a new set of period-absolute magnitude-metallicity (PMZ) relations for single-mode RR Lyrae stars calibrated for the optical GBP, V, G, GRP, near-infrared I, J, H, and Ks passbands. We compiled a large dataset (over 100 objects) of fundamental and first-overtone RR Lyrae pulsators consisting of mean inte…

2024 Astronomy and Astrophysics
Gaia 13
The first degree-scale starlight-polarization-based tomography map of the magnetized interstellar medium
DOI: 10.1051/0004-6361/202349015 Bibcode: 2024A&A...684A.162P

Eriksen, H. K.; Ghosh, T.; Gjerløw, E. +21 more

We present the first degree-scale tomography map of the dusty magnetized interstellar medium (ISM) from stellar polarimetry and distance measurements. We used the RoboPol polarimeter at Skinakas Observatory to conduct a survey of the polarization of starlight in a region of the sky of about four square degrees. We propose a Bayesian method to deco…

2024 Astronomy and Astrophysics
Gaia 13
CARMENES input catalog of M dwarfs. VII. New rotation periods for the survey stars and their correlations with stellar activity
DOI: 10.1051/0004-6361/202346794 Bibcode: 2024A&A...684A...9S

Nagel, E.; Amado, P. J.; Caballero, J. A. +40 more


Aims: Knowledge of rotation periods (Prot) is important for understanding the magnetic activity and angular momentum evolution of late-type stars, as well as for evaluating radial velocity signals of potential exoplanets and identifying false positives. We measured photometric and spectroscopic Prot for a large sample of…

2024 Astronomy and Astrophysics
Gaia 13
Correlation between accretion rate and free-free emission in protoplanetary disks. A multiwavelength analysis of central mm/cm emission in transition disks
DOI: 10.1051/0004-6361/202348387 Bibcode: 2024A&A...684A.134R

van der Marel, N.; van der Tak, F. F. S.; Francis, L. +3 more

Context. The inner regions of protoplanetary disks are believed to be the primary locations of planet formation and the processes that influence the global evolution of the disk, such as magnetohydrodynamic winds and photoevaporation. Transition disks with large inner dust cavities are ideal targets for studying the inner regions (of tens of au) o…

2024 Astronomy and Astrophysics
Gaia 13
Imaging dark matter at the smallest scales with z ≈ 1 lensed stars
DOI: 10.1051/0004-6361/202450474 Bibcode: 2024A&A...689A.167D

Koekemoer, Anton M.; Treu, Tommaso; Filippenko, Alexei V. +19 more

Recent observations of caustic-crossing galaxies at redshift 0.7 ≲ z ≲ 1 show a wealth of transient events. Most of them are believed to be microlensing events of highly magnified stars. Earlier work predicts such events should be common near the critical curves (CCs) of galaxy clusters ("near region"), but some are found relatively far away from …

2024 Astronomy and Astrophysics
eHST 13
The metal-poor edge of the Milky Way's "thin disc"
DOI: 10.1051/0004-6361/202348918 Bibcode: 2024A&A...685A.151F

Sestito, Federico; Martin, Nicolas; Kordopatis, Georges +9 more

Context. The emergence of the disc in our Galaxy and the relation between thick and thin disc formation and evolution is still a matter of debate. The chemo-dynamical characterization of disc stars is key to resolving this question, particularly at parameter regimes, where both disc components overlap, such as the region around [Fe/H] ∼ −0.7 corre…

2024 Astronomy and Astrophysics
Gaia 13