Search Publications

The search for DA double white dwarf binary candidates from SDSS DR14
DOI: 10.1051/0004-6361/202347617 Bibcode: 2024A&A...684A.103Y

Zhao, Gang; Li, Zhenwei; Zhao, Jingkun +4 more


Aims: Double white dwarf (DWD) binaries are one of the channels through which type Ia supernovae explosions occur. With the release of more and more sky survey data, the search for additional DWDs has become a possibility. We utilized the spectroscopic data from SDSS DR14 to search for DWD binaries based on variations in radial velocities (RV…

2024 Astronomy and Astrophysics
Gaia 1
Flare heating of the chromosphere: Observations of flare continuum from GREGOR and IRIS
DOI: 10.1051/0004-6361/202451219 Bibcode: 2024A&A...690A.254G

Berlicki, A.; Liu, W.; Dudík, J. +8 more

Context. On 2022 May 4, an M5.7 flare erupted in the active region NOAA 13004, which was the target of a coordinated campaign between GREGOR, IRIS, Hinode, and ground-based instruments at the Ondřejov observatory. A flare kernel located at the edge of a pore was co-observed by the IRIS slit and GREGOR HiFI+ imagers. Aims. We investigated the flare…

2024 Astronomy and Astrophysics
IRIS 1
Multi-spacecraft study with the Icarus model: Modelling the propagation of CMEs to Mercury and Earth
DOI: 10.1051/0004-6361/202450430 Bibcode: 2024A&A...689A..98B

Schmieder, B.; Poedts, S.; Démoulin, P. +2 more

Context. Coronal mass ejections (CMEs) are the main drivers of the disturbances in interplanetary space. Earth-directed CMEs can be dangerous, and understanding the CME interior magnetic structure is crucial for advancing space weather studies. It is important to assess the capabilities of a numerical heliospheric model, as a firm understanding of…

2024 Astronomy and Astrophysics
SOHO 1
Lithium, rotation and metallicity in the open cluster M35
DOI: 10.1051/0004-6361/202450222 Bibcode: 2024A&A...687A.234C

Bouy, H.; Barrado, D.; Agüeros, M. A. +2 more

Context. Lithium (Li) abundance is an age indicator for G, K, and M stellar types, as its abundance decreases over time for these spectral types. However, despite all of the observational efforts made over the past few decades, the role of rotation, stellar activity, and metallicity in the depletion of Li is still unclear.
Aims: Our purpose i…

2024 Astronomy and Astrophysics
Gaia 1
Stellar halo density with LAMOST K and M giants
DOI: 10.1051/0004-6361/202348781 Bibcode: 2024A&A...684A.135L

Wang, H. -F.; López-Corredoira, M.; Liu, C. +3 more


Aims: We derive the morphology of the stellar component in the outer halo volume, and search for possible overdensities due to substructures therein.
Methods: We made use of some of the data releases of the spectroscopic survey LAMOST DR8-DR9 in tandem with distance determinations for two subsamples, that is, of K-giants and M-giants, re…

2024 Astronomy and Astrophysics
Gaia 1
Properties of flare events based on light curves from the TESS survey: II. 20-second cadence
DOI: 10.1051/0004-6361/202348343 Bibcode: 2024A&A...689A.103Z

Zhang, Liyun; Han, Xianming L.; Misra, Prabhakar +2 more

Aims. Stellar flares are sudden bursts of energy and are the result of magnetic activity. We used light curves from the TESS 20-second cadence survey from 2020 to 2023 to detect flare events and determine their properties. Methods. By means of repeated fitting to distinguish stellar background light curves and flare events, we detected 32 978 flar…

2024 Astronomy and Astrophysics
Gaia 1
A halo model approach to describe clustering and emission of the two main star-forming galaxy populations for cosmic infrared background studies
DOI: 10.1051/0004-6361/202451424 Bibcode: 2024A&A...692A.190Z

Calabrese, E.; Pagano, L.; Negrello, M. +3 more

The cosmic infrared background (CIB), which is traced by the emission from dusty star-forming galaxies, provides a crucial window into the phases of star formation throughout cosmic history. These galaxies, although challenging to detect individually at high redshifts due to their faintness, cumulatively contribute to the CIB, which then becomes a…

2024 Astronomy and Astrophysics
Herschel 1
J-PLUS: The fraction of calcium white dwarfs along the cooling sequence
DOI: 10.1051/0004-6361/202451226 Bibcode: 2024A&A...691A.211L

Hernández-Monteagudo, C.; Hernán-Caballero, A.; Gänsicke, B. T. +24 more

Aims. We used the Javalambre Photometric Local Universe Survey (J-PLUS) second data release (DR2) photometry in 12 optical bands over 2176 deg2 to estimate the fraction of white dwarfs with the presence of Ca II H+K absorption along the cooling sequence. Methods. We compared the J-PLUS photometry against metal-free theoretical models to…

2024 Astronomy and Astrophysics
Gaia 1
Gaia DR3 reveals the complex dynamical evolution within star clusters
DOI: 10.1051/0004-6361/202450573 Bibcode: 2024A&A...689A.268V

Miret-Roig, N.; Randich, S.; Alves, J. +6 more

Context. Star clusters, composed of stars born from the same molecular cloud, serve as invaluable natural laboratories for understanding the fundamental processes governing stellar formation and evolution. Aims. This study aims to investigate correlations between the Mean Interdistance ($ \bar{D_{\ma…

2024 Astronomy and Astrophysics
Gaia 1
Compositional characterization of a primordial S-type asteroid family of the inner main belt
DOI: 10.1051/0004-6361/202347391 Bibcode: 2024A&A...682A..64B

Fornasier, S.; Delbo, M.; Ochner, P. +4 more

Context. Recently, a primordial family of moderate-albedo asteroid fragments was discovered in the inner main belt. Its age was estimated to be 4.4 ± 1.7 Gyr. However, there is a lack of compositional characterization, which is important to the study of the earliest collisions in the main belt.
Aims: In addition to the previously identified m…

2024 Astronomy and Astrophysics
Gaia 1