Search Publications

Runaways and shells around the CMa OB1 association
DOI: 10.1051/0004-6361/201935484 Bibcode: 2019A&A...628A..44F

Montmerle, T.; Gregorio-Hetem, J.; Santos-Silva, T. +1 more

Context. The origin of the arc-shaped Sh 2-296 nebula is still unclear. Mainly due to its morphology, the nebula has been suggested to be a 0.5 Myr old supernova remnant (SNR) that could be inducing star formation in the CMa OB1 association. This means that the region might be an excellent laboratory for investigating the influence of massive star…

2019 Astronomy and Astrophysics
AKARI Gaia 13
Multi-waveband detection of quasi-periodic pulsations in a stellar flare on EK Draconis observed by XMM-Newton
DOI: 10.1051/0004-6361/201935653 Bibcode: 2019A&A...629A.147B

Broomhall, A. -M.; Rosen, S. R.; Pye, J. P. +2 more

Context. Quasi-periodic pulsations (QPPs) are time variations in the energy emission during a flare that are observed on both the Sun and other stars and thus have the potential to link the physics of solar and stellar flares.
Aims: We characterise the QPPs detected in an X-ray flare on the solar analogue, EK Draconis, which was observed by X…

2019 Astronomy and Astrophysics
Gaia XMM-Newton 13
SHALOS: Statistical Herschel-ATLAS lensed objects selection
DOI: 10.1051/0004-6361/201935475 Bibcode: 2019A&A...627A..31G

Bonavera, L.; González-Nuevo, J.; Herranz, D. +7 more

Context. The statistical analysis of large sample of strong lensing events can be a powerful tool to extract astrophysical or cosmological valuable information. Their selection using submillimetre galaxies has been demonstrated to be very effective with more than ∼200 proposed candidates in the case of Herschel-ATLAS data and several tens in the c…

2019 Astronomy and Astrophysics
Herschel 13
Vertical position of the Sun with γ-rays
DOI: 10.1051/0004-6361/201936659 Bibcode: 2019A&A...632L...1S

Siegert, Thomas

We illustrate a method for estimating the vertical position of the Sun above the Galactic plane by γ-ray observations. Photons of γ-ray wavelengths are particularly well suited for geometrical and kinematic studies of the Milky Way because they are not subject to extinction by interstellar gas or dust. Here, we use the radioactive decay line of

2019 Astronomy and Astrophysics
INTEGRAL 13
MUSE-AO view of the starburst-AGN connection: NGC 7130
DOI: 10.1051/0004-6361/201834669 Bibcode: 2019A&A...621L...5K

Knapen, J. H.; Comerón, S.; Seidel, M. K.

We present the discovery of a small kinematically decoupled core of 0.″2 (60 pc) in radius as well as an outflow jet in the archetypical AGN-starburst "composite" galaxy NGC 7130 from integral field data obtained with the adaptive optics-assisted MUSE-NFM instrument on the VLT. Correcting the already good natural seeing at the time of our science …

2019 Astronomy and Astrophysics
Gaia eHST 13
Solar wind charge exchange in cometary atmospheres. I. Charge-changing and ionization cross sections for He and H particles in H2O
DOI: 10.1051/0004-6361/201834848 Bibcode: 2019A&A...630A..35S

Alho, Markku; Simon Wedlund, Cyril; Nilsson, Hans +7 more

Context. Solar wind charge-changing reactions are of paramount importance to the physico-chemistry of the atmosphere of a comet, mass-loading the solar wind through an effective conversion of fast light solar wind ions into slow heavy cometary ions.
Aims: To understand these processes and place them in the context of a solar wind plasma inter…

2019 Astronomy and Astrophysics
Rosetta 13
Observations of solar small-scale magnetic flux-sheet emergence
DOI: 10.1051/0004-6361/201834628 Bibcode: 2019A&A...622L..12F

Bello González, N.; Borrero, J. M.; Fischer, C. E. +1 more


Aims: Two types of flux emergence were recently discovered in numerical simulations: magnetic loops and magnetic sheet emergence. While magnetic loop emergence has been documented well in recent years using high-resolution full Stokes data from ground-based telescopes as well as satellites, magnetic sheet emergence is still an understudied pr…

2019 Astronomy and Astrophysics
Hinode 13
The CEMP star SDSS J0222-0313: the first evidence of proton ingestion in very low-metallicity AGB stars?
DOI: 10.1051/0004-6361/201935680 Bibcode: 2019A&A...628A..46C

Salvadori, S.; Bonifacio, P.; Caffau, E. +9 more

Context. Carbon-enhanced metal-poor (CEMP) stars are common objects in the metal-poor regime. The lower the metallicity we look at, the larger the fraction of CEMP stars with respect to metal-poor stars with no enhancement in carbon. The chemical pattern of CEMP stars is diversified, strongly suggesting a different origin of the C enhancement in t…

2019 Astronomy and Astrophysics
Gaia 13
Searching for g modes. II. Unconfirmed g-mode detection in the power spectrum of the time series of round-trip travel time
DOI: 10.1051/0004-6361/201935196 Bibcode: 2019A&A...624A.106A

Corbard, T.; Appourchaux, T.

Context. The recent claims of g-mode detection have restarted the search for these potentially extremely important modes. The claimed detection of g modes was obtained from the analysis of the power spectrum of the time series of round-trip travel time of p modes.
Aims: The goal of this paper is to reproduce these results on which the claims …

2019 Astronomy and Astrophysics
SOHO 13
Peering at the outflow mechanisms in the transitional pulsar PSR J1023+0038: simultaneous VLT, XMM-Newton, and Swift high-time resolution observations
DOI: 10.1051/0004-6361/201936008 Bibcode: 2019A&A...631A.104B

D'Avanzo, P.; Campana, S.; Casella, P. +6 more

We report on a simultaneous near-infrared, optical, and X-ray campaign performed in 2017 with the XMM-Newton and Swift satellites and the HAWK-I instrument mounted on the Very Large Telescope (VLT) on the transitional millisecond pulsar PSR J1023+0038. Near-infrared observations were performed in fast-photometric mode (0.5 s exposure time) in orde…

2019 Astronomy and Astrophysics
XMM-Newton 13