Search Publications

A soft and transient ultraluminous X-ray source with six-hour modulation in the NGC 300 galaxy
DOI: 10.1051/0004-6361/202346463 Bibcode: 2024A&A...682A.151S

Tiengo, A.; de Martino, D.; Pinto, C. +13 more

We investigate the nature of CXOU J005440.5−374320 (J0054), a peculiar bright (∼4 × 1039 erg s−1) and soft X-ray transient in the spiral galaxy NGC 300 with a six-hour periodic flux modulation that was detected in a 2014 Chandra observation. Subsequent observations with Chandra and XMM-Newton, as well as a large observational…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 0
Reconciling concentration to virial mass relations
DOI: 10.1051/0004-6361/202451220 Bibcode: 2024A&A...691A.362L

Saha, Prasenjit; Ferreras, Ignacio; Leier, Dominik +1 more

Context. The concentration-virial mass (c-M) relation is a fundamental scaling relation within the standard cold dark matter (ΛCDM) framework well established in numerical simulations. However, observational constraints of this relation are hampered by the difficulty of characterising the properties of dark matter haloes. Recent comparisons betwee…

2024 Astronomy and Astrophysics
eHST 0
Evolution of BD-14 3065b (TOI-4987b) from giant planet to brown dwarf as possible evidence of deuterium burning at old stellar ages
DOI: 10.1051/0004-6361/202349028 Bibcode: 2024A&A...688A.120S

Latham, David W.; Quinn, Samuel N.; Berlind, Perry +20 more

The present study confirms BD-14 3065b as a transiting planet-brown dwarf in a triple-star system, with a mass near the deuterium-burning boundary. BD-14 3065b has the largest radius observed within the sample of giant planets and brown dwarfs around post-main sequence stars. Its orbital period is 4.3 days and it transits a subgiant F-type star wi…

2024 Astronomy and Astrophysics
Gaia 0
Revealing the inner workings of the lensed quasar SDSS J1339+1310: Insights from microlensing analysis
DOI: 10.1051/0004-6361/202450151 Bibcode: 2024A&A...689A.129F

Kaspi, S.; Muñoz, J. A.; Mediavilla, E. +4 more

Aims. We aim to unveil the structure of the continuum and broad-emission line (BEL) emitting regions in the gravitationally lensed quasar SDSS J1339+1310 by examining the distinct signatures of microlensing present in this system. Our study involves a comprehensive analysis of ten years (2009–2019) of photometric monitoring data and seven spectros…

2024 Astronomy and Astrophysics
eHST 0
Abundance of strontium in the Galactic globular cluster 47 Tuc
DOI: 10.1051/0004-6361/202347936 Bibcode: 2024A&A...682A.126K

Kučinskas, A.; Kolomiecas, E.; Dobrovolskas, V. +1 more


Aims: We have determined Sr abundance in a sample of 31 red giant branch stars located in the Galactic globular cluster 47 Tuc with the aim to identify potential differences in the Sr abundance between first population (1P, Na-poor) and second population (2P, Na-rich) stars.
Methods: We derived the Na and Sr abundances from the archival …

2024 Astronomy and Astrophysics
Gaia 0
The accreted galaxy: An overview of TESS metal-poor accreted star candidates
DOI: 10.1051/0004-6361/202450610 Bibcode: 2024A&A...690A.120D

Hawkins, Keith; Jofré, Paula; de Brito Silva, Danielle +2 more

The Milky Way is a mosaic of stars from different origins. In particular, metal-poor accreted star candidates offer a unique opportunity to better understand the accretion history of the Milky Way. In this work, we aim to explore the assembly history of the Milky Way by investigating accreted stars in terms of their ages, dynamical properties, and…

2024 Astronomy and Astrophysics
Gaia 0
Revisiting the massive star-forming complex RCW 122: New millimeter and submillimeter study
DOI: 10.1051/0004-6361/202349136 Bibcode: 2024A&A...689A..76D

Baume, G.; Gamen, R.; Merello, M. +9 more

In this paper, we present a new multifrequency study of the giant star-forming complex RCW 122. We used molecular data obtained with the ASTE 10 m and the APEX 12 m telescopes, along with infrared observations spanning from 3.6 µm to 870 µm, obtained from available databases. We also incorporated a range of public datasets, including the radio con…

2024 Astronomy and Astrophysics
Herschel 0
Different manifestations of a loop-like transient brightening in solar atmospheres
DOI: 10.1051/0004-6361/202449396 Bibcode: 2024A&A...691A.309C

Wang, Jincheng; Cai, Qiangwei; Feng, Hengqiang +1 more

Context. Small-scale transient brightenings that are the consequence of magnetic reconnection play pivotal roles in the heating process of solar atmospheres. These phenomena contain key information about the dynamic evolution of the solar magnetic field. The fine-scale structures triggered by instabilities in these brightenings are intimately conn…

2024 Astronomy and Astrophysics
IRIS 0
Faint mm NIKA2 dusty star-forming galaxies: Finding the high-redshift population
DOI: 10.1051/0004-6361/202243887 Bibcode: 2024A&A...683A.232B

Berta, S.; Aussel, H.; Adam, R. +46 more


Aims: High-redshift dusty star-forming galaxies (DSFGs) are proposed to be the progenitors of massive quiescent galaxies arising at cosmic noon, providing a crucial insight into the formation, assembly, and early quenching of massive galaxies in the early Universe. However, their high redshift combined with high dust obscuration adds signific…

2024 Astronomy and Astrophysics
Herschel 0
Stellar chromospheric activity database of solar-like stars based on the LAMOST Low-Resolution Spectroscopic Survey. II. The bolometric and photospheric calibration
DOI: 10.1051/0004-6361/202348988 Bibcode: 2024A&A...688A..23Z

Zhang, Jun; Zhang, Haotong; Luo, Ali +2 more

Context. The dependence of stellar magnetic activity on stellar parameters is inspired by the chromospheric activity studies based on the large-scale spectroscopic surveys.
Aims: The main objective of this project is to provide the chromospheric activity parameter database for the LAMOST Low-Resolution Spectroscopic Survey (LRS) spectra of so…

2024 Astronomy and Astrophysics
Gaia 0