Search Publications

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
Unusually high magnetic fields in the coma of 67P/Churyumov-Gerasimenko during its high-activity phase
DOI: 10.1051/0004-6361/201833544 Bibcode: 2019A&A...630A..38G

Tsurutani, B. T.; Behar, E.; Nilsson, H. +10 more


Aims: On July 3, 2015, an unprecedented increase in the magnetic field magnitude was measured by the Rosetta spacecraft orbiting comet 67P/Churyumov-Gerasimenko (67P). This increase was accompanied by large variations in magnetic field and ion and electron density and energy. To our knowledge, this unusual event marks the highest magnetic fie…

2019 Astronomy and Astrophysics
Rosetta 13
Flow pattern of accelerated cometary ions inside and outside the diamagnetic cavity of comet 67P/Churyumov-Gerasimenko
DOI: 10.1051/0004-6361/201935122 Bibcode: 2019A&A...630A..43M

Behar, E.; Nilsson, H.; Goetz, C. +3 more

Analyzing data from the Ion Composition Analyzer on board the Rosetta spacecraft, we studied a flow pattern of accelerated cometary ions (40-80 eV) inside and outside the diamagnetic cavity of comet 67P/Churyumov-Gerasimenko (67P). We found that the accelerated ions are intermittently observed and are ten times more frequently observed outside the…

2019 Astronomy and Astrophysics
Rosetta 13
IRAM and Gaia views of multi-episodic star formation in IC 1396A. The origin and dynamics of the Class 0 protostar at the edge of an HII region
DOI: 10.1051/0004-6361/201833207 Bibcode: 2019A&A...622A.118S

Fang, Min; Sicilia-Aguilar, Aurora; Roccatagliata, Veronica +3 more

Context. IC 1396A is a cometary globule that contains the Class 0 source IC 1396A-PACS-1, which was discovered with Herschel.
Aims: We use IRAM 30m telescope and Gaia DR2 data to explore the star formation history of IC 1396A and investigate the possibilities of triggered star formation.
Methods: IRAM and Herschel continuum data were use…

2019 Astronomy and Astrophysics
Gaia Herschel 13
IC 4665 DANCe. I. Members, empirical isochrones, magnitude distributions, present-day system mass function, and spatial distribution
DOI: 10.1051/0004-6361/201935518 Bibcode: 2019A&A...631A..57M

Tamura, M.; Bertin, E.; Miret-Roig, N. +12 more

Context. The study of star formation is extremely challenging, due to the lack of complete and clean samples of young nearby clusters and star-forming regions. The recent Gaia DR2 catalogue complemented with the deep ground-based COSMIC DANCe catalogue offers a new database of unprecedented accuracy to revisit the membership of clusters and star-f…

2019 Astronomy and Astrophysics
Gaia 13
Star-forming galaxies at low-redshift in the SHARDS survey
DOI: 10.1051/0004-6361/201731670 Bibcode: 2019A&A...621A..52L

Mas-Hesse, J. M.; Hernán-Caballero, A.; Koekemoer, A. M. +13 more

Context. The physical processes driving the evolution of star formation (SF) in galaxies over cosmic time still present many open questions. Recent galaxy surveys allow now to study these processes in great detail at intermediate redshift (0 ≤ z ≤ 0.5).
Aims: We build a complete sample of star-forming galaxies and analyze their properties, re…

2019 Astronomy and Astrophysics
eHST 13
LMC S154: the first Magellanic symbiotic recurrent nova
DOI: 10.1051/0004-6361/201834165 Bibcode: 2019A&A...624A.133I

Gromadzki, Mariusz; Miszalski, Brent; Iłkiewicz, Krystian +3 more

Classical nova outburst has been suggested for a number of extragalactic symbiotic stars, but in none of the systems has it been proven. In this work we study the nature of one of these systems, LMC S154. We gathered archival photometric observations in order to determine the timescales and nature of variability in this system. Additionally we car…

2019 Astronomy and Astrophysics
AKARI IUE 12