Search Publications

Pulsating hydrogen-deficient white dwarfs and pre-white dwarfs observed with TESS. II. Discovery of two new GW Vir stars: TIC 333432673 and TIC 095332541
DOI: 10.1051/0004-6361/202141253 Bibcode: 2021A&A...655A..27U

Werner, K.; Kepler, S. O.; Althaus, L. G. +8 more

Context. The Transiting Exoplanet Survey Satellite (TESS) mission is revolutionizing the blossoming area of asteroseismology, particularly of pulsating white dwarfs and pre-white dwarfs, thus continuing the impulse of its predecessor, the Kepler mission.
Aims: In this paper, we present the observations from the extended TESS mission in both 1…

2021 Astronomy and Astrophysics
Gaia 13
Observations of a prominence eruption and loop contraction
DOI: 10.1051/0004-6361/202040042 Bibcode: 2021A&A...647A..85D

Joshi, Bhuwan; Schmieder, Brigitte; Joshi, Reetika +3 more

Context. Prominence eruptions provide key observations to understand the launch of coronal mass ejections as their cold plasma traces a part of the unstable magnetic configuration.
Aims: We select a well observed case to derive observational constraints for eruption models.
Methods: We analyze the prominence eruption and loop expansion a…

2021 Astronomy and Astrophysics
SOHO 13
Simultaneous X-ray and radio observations of the transitional millisecond pulsar candidate CXOU J110926.4-650224. The discovery of a variable radio counterpart
DOI: 10.1051/0004-6361/202141431 Bibcode: 2021A&A...655A..52C

Campana, S.; de Martino, D.; Rea, N. +15 more

We present the results of simultaneous observations of the transitional millisecond pulsar (tMSP) candidate CXOU J110926.4-650224 with the XMM-Newton satellite and the MeerKAT telescope. The source was found at an average X-ray luminosity of LX ≃ 7 × 1033 erg s−1 over the 0.3−10 keV band (assumin…

2021 Astronomy and Astrophysics
Gaia XMM-Newton 13
The RR Lyrae projected density distribution from the Galactic centre to the halo
DOI: 10.1051/0004-6361/202038463 Bibcode: 2021A&A...646A..45N

Minniti, Dante; Ripepi, Vincenzo; Alonso-García, Javier +4 more

The projected density distribution of type ab RR Lyrae (RRab) stars was characterised from the innermost regions of the Milky Way to the halo, with the aim of placing constraints on the Galaxy's evolution. The compiled sample (NRRab = 64 850) stems from fundamental mode RR Lyrae variables identified by the VVV, OGLE, and Gaia surveys. T…

2021 Astronomy and Astrophysics
Gaia 13
The Fornax3D project: Planetary nebulae catalogue and independent distance measurements to Fornax cluster galaxies
DOI: 10.1051/0004-6361/202141314 Bibcode: 2021A&A...653A.167S

Viaene, S.; Morelli, L.; Pinna, F. +17 more

Extragalactic planetary nebulae (PNe) offer a way to determine the distance to their host galaxies thanks to the nearly universal shape of the planetary nebulae luminosity function (PNLF). Accurate PNe distance measurements rely on obtaining well-sampled PNLFs and the number of observed PNe scales with the encompassed stellar mass. This means eith…

2021 Astronomy and Astrophysics
eHST 13
Determining the source and eruption dynamics of a stealth CME using NLFFF modelling and MHD simulations
DOI: 10.1051/0004-6361/202141142 Bibcode: 2021A&A...652A.160Y

Yardley, S. L.; Pagano, P.; Mackay, D. H. +1 more

Context. Coronal mass ejections (CMEs) that exhibit weak or no eruption signatures in the low corona, known as stealth CMEs, are problematic as upon arrival at Earth they can lead to geomagnetic disturbances that were not predicted by space weather forecasters.
Aims: We investigate the origin and eruption of a stealth event that occurred on 2…

2021 Astronomy and Astrophysics
SOHO 13
The variable absorption in the X-ray spectrum of GRB 190114C
DOI: 10.1051/0004-6361/202140439 Bibcode: 2021A&A...649A.135C

Perna, Rosalba; Campana, Sergio; Lazzati, Davide +2 more

Gamma-ray burst (GRB) 190114C was a bright burst that occurred in the local Universe (z = 0.425). It was the first GRB ever detected at teraelectronvolt (TeV) energies, and this was thanks to MAGIC. We characterize the ambient medium properties of the host galaxy through the study of the absorbing X-ray column density. Using a combination of Swift…

2021 Astronomy and Astrophysics
XMM-Newton 13
Towards a fully consistent Milky Way disk model. IV. The impact of Gaia DR2 and APOGEE
DOI: 10.1051/0004-6361/202038840 Bibcode: 2021A&A...647A..39S

Just, A.; Sysoliatina, K.


Aims: We present an updated version of the semi-analytic Just-Jahrei (JJ) model of the Galactic disk and constrain its parameters in the Solar neighbourhood.
Methods: The new features of the JJ model include a simple two-component gaseous disk, a star-formation rate (SFR) function of the thick disk that has been extended in time, and a c…

2021 Astronomy and Astrophysics
Gaia 13
Description of turbulent dynamics in the interstellar medium: multifractal-microcanonical analysis. I. Application to Herschel observations of the Musca filament
DOI: 10.1051/0004-6361/202039874 Bibcode: 2021A&A...649A..33Y

Schneider, N.; Bontemps, S.; Elia, D. +10 more

Observations of the interstellar medium (ISM) show a complex density and velocity structure, which is in part attributed to turbulence. Consequently, the multifractal formalism should be applied to observation maps of the ISM in order to characterize its turbulent and multiplicative cascade properties. However, the multifractal formalism, even in …

2021 Astronomy and Astrophysics
Gaia Herschel 13
Four Jovian planets around low-luminosity giant stars observed by the EXPRESS and PPPS
DOI: 10.1051/0004-6361/202038555 Bibcode: 2021A&A...646A.131J

Jones, M. I.; Trifonov, T.; Soto, M. G. +14 more

We report the discovery of planetary companions orbiting four low-luminosity giant stars with M between 1.04 and 1.39 M. All four host stars have been independently observed by the EXoPlanets aRound Evolved StarS (EXPRESS) program and the Pan-Pacific Planet Search (PPPS). The companion signals were revealed by multi-epoch p…

2021 Astronomy and Astrophysics
Gaia 13