Search Publications

Observations of GRO J1744-28 in quiescence with XMM-Newton
DOI: 10.1051/0004-6361/202038093 Bibcode: 2020A&A...643A..62D

Tsygankov, S.; Santangelo, A.; Doroshenko, V. +3 more

We report on the deep observations of the "bursting pulsar" GRO J1744-28, which were performed with XMM-Newton and aimed to clarify the origin of its X-ray emission in quiescence. We detect the source at a luminosity level of ∼1034 erg s-1 with an X-ray spectrum that is consistent with the power law, blackbody, or accretion-h…

2020 Astronomy and Astrophysics
Gaia XMM-Newton 9
An accurate strong lensing model of the Abell 2163 core
DOI: 10.1051/0004-6361/201936590 Bibcode: 2020A&A...635A..98R

Grillo, C.; Rosati, P.; Lombardi, M. +6 more

Abell 2163 at z ≃ 0.201 is one of the most massive galaxy clusters known, very likely in a post-merging phase. Data from several observational windows suggest a complex mass structure with interacting subsystems, which makes the reconstruction of a realistic merging scenario very difficult. A missing key element in this sense is unveiling the clus…

2020 Astronomy and Astrophysics
eHST 9
Benchmarking the fundamental parameters of Ap stars with optical long-baseline interferometric measurements
DOI: 10.1051/0004-6361/202038753 Bibcode: 2020A&A...642A.101P

Shulyak, D.; Ryabchikova, T.; Meilland, A. +10 more

Context. The variety of physical processes at play in chemically peculiar stars makes it difficult to determine their fundamental parameters. In particular, for the magnetic ones, called Ap stars, the strong magnetic fields and the induced spotted stellar surfaces may lead to biased effective temperatures when these values are derived through spec…

2020 Astronomy and Astrophysics
Gaia IUE 9
Detailed abundances in a sample of very metal-poor stars
DOI: 10.1051/0004-6361/202038028 Bibcode: 2020A&A...642A..25F

Bonifacio, P.; Caffau, E.; Spite, M. +6 more

Context. Unevolved metal-poor stars bore witness to the early evolution of the Galaxy, and the determination of their detailed chemical composition is an important tool to understand its chemical history. The study of their chemical composition can also be used to constrain the nucleosynthesis of the first generation of supernovae that enriched th…

2020 Astronomy and Astrophysics
Gaia 9
Kinematics of coronal mass ejections in the LASCO field of view
DOI: 10.1051/0004-6361/202037834 Bibcode: 2020A&A...639A..68R

Yashiro, Seiji; Ravishankar, Anitha; Michałek, Grzegorz

In this paper we present a statistical study of the kinematics of 28894 coronal mass ejections (CMEs) recorded by the Large Angle and Spectrometric Coronagraph (LASCO) on board the Solar and Heliospheric Observatory spacecraft from 1996 until mid-2017. The initial acceleration phase is characterized by a rapid increase in CME velocity just after e…

2020 Astronomy and Astrophysics
SOHO 9
High-precision calculation of the light curve and its interpretation
DOI: 10.1051/0004-6361/201936731 Bibcode: 2020A&A...633A..96A

Abubekerov, M. K.; Gostev, N. Yu.

We present a highly precise calculation of the theoretical light curve and its derivatives for a binary star-planet system in an elliptical orbit. We also describe an analytical fitting by limb-darkening coefficients to reduce the number of parameters for nonlinear fitting. We demonstrate the practical importance of the precision computation of th…

2020 Astronomy and Astrophysics
eHST 9
Ground-based visible spectroscopy of asteroids to support the development of an unsupervised Gaia asteroid taxonomy
DOI: 10.1051/0004-6361/202038246 Bibcode: 2020A&A...642A..80C

Tanga, P.; Galluccio, L.; Cellino, A. +4 more

Context. The Gaia mission of the European Space Agency is measuring reflectance spectra of a number to the order of 105 small Solar System objects. A first sample will be published in the Gaia Data Release scheduled for 2021.
Aims: The aim of our work was to test the procedure developed to obtain taxonomic classifications for aster…

2020 Astronomy and Astrophysics
Gaia 9
Pulsational properties of ten new slowly pulsating B stars
DOI: 10.1051/0004-6361/201935478 Bibcode: 2020A&A...633A.122F

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

Context. Slowly pulsating B (SPB) stars are upper main-sequence multi-periodic pulsators that show non-radial g-mode oscillations driven by the κ mechanism acting on the iron bump. These multi-periodic pulsators have great asteroseismic potential and can be employed for the calibration of stellar structure and evolution models of massive stars.

2020 Astronomy and Astrophysics
Gaia INTEGRAL 9
Feedback of molecular outflows from protostars in NGC 1333 revealed by Herschel and Spitzer spectro-imaging observations
DOI: 10.1051/0004-6361/202037684 Bibcode: 2020A&A...641A..36D

Güdel, Manuel; Persson, Magnus; Tafalla, Mario +2 more

Context. Far infrared cooling of excited gas around protostars has been predominantly studied in the context of pointed observations. Large-scale spectral maps of star forming regions enable the simultaneous, comparative study of the gas excitation around an ensemble of sources at a common frame of reference, therefore, providing direct insights i…

2020 Astronomy and Astrophysics
Herschel 9
Component properties and mutual orbit of binary main-belt comet 288P/(300163) 2006 VW139
DOI: 10.1051/0004-6361/202038195 Bibcode: 2020A&A...643A.152A

Agarwal, J.; Weaver, H.; Larson, S. +3 more

Context. The binary asteroid 288P/(300163) is unusual both for its combination of wide-separation and high mass ratio and for its comet-like activity. It is not currently known whether there is a causal connection between the activity and the unusual orbit or if instead the activity helped to overcome a strong detection bias against such sub-arcse…

2020 Astronomy and Astrophysics
eHST 9