Search Publications

Structure of sunspot light bridges in the chromosphere and transition region
DOI: 10.1051/0004-6361/201629828 Bibcode: 2018A&A...609A..73R

Rezaei, R.

Context. Light bridges (LBs) are elongated structures with enhanced intensity embedded in sunspot umbra and pores.
Aims: We studied the properties of a sample of 60 LBs observed with the Interface Region Imaging Spectrograph (IRIS).
Methods: Using IRIS near- and far-ultraviolet spectra, we measured the line intensity, width, and Doppler …

2018 Astronomy and Astrophysics
IRIS 9
Discovery of large scale shock fronts correlated with the radio halo and radio relic in the A2163 galaxy cluster
DOI: 10.1051/0004-6361/201834053 Bibcode: 2018A&A...619A..68T

Thölken, Sophia; Reiprich, Thomas H.; Ota, Naomi +1 more

Context. Galaxy clusters form at the intersections of the filamentary large scale structure in merging events and by the accretion of matter along these filaments. Imprints of these formation processes should be visible in the intracluster medium and can arise in shock fronts, which are detectable via discontinuities in, for example, the gas tempe…

2018 Astronomy and Astrophysics
Suzaku XMM-Newton 9
Solving non-LTE problems in rotational transitions using the Gauss-Seidel method and its implementation in the Atmospheric Radiative Transfer Simulator
DOI: 10.1051/0004-6361/201833566 Bibcode: 2018A&A...619A.181Y

Hartogh, P.; Yamada, T.; Rezac, L. +3 more

This article presents our implementation of a non-LTE solver in spherical symmetry for molecular rotational transition in static or expanding atmospheres. The new open-source code relies on the Gauss-Seidel Accelerated Lambda Iteration methodology that provides a rapid and accurate convergence of the non-LTE problems, which is now routinely used i…

2018 Astronomy and Astrophysics
Rosetta 8
PACS and SPIRE range spectroscopy of cool, evolved stars
DOI: 10.1051/0004-6361/201833168 Bibcode: 2018A&A...618A.143N

Decin, L.; Lombaert, R.; Groenewegen, M. A. T. +3 more

Context. At the end of their lives AGB stars are prolific producers of dust and gas. The details of this mass-loss process are still not understood very well. Herschel PACS and SPIRE spectra which cover the wavelength range from ∼55 to 670 µm almost continuously, offer a unique way of investigating properties of AGB stars in general and the …

2018 Astronomy and Astrophysics
Herschel 8
The long-period massive binary HD 54662 revisited
DOI: 10.1051/0004-6361/201732095 Bibcode: 2018A&A...615A..19M

Rauw, G.; Mahy, L.; Mossoux, E.

Context. HD 54662 is an O-type binary star belonging to the CMa OB1 association. Because of its long-period orbit, this system is an interesting target to test the adiabatic wind shock model.
Aims: The goal of this study is to improve our knowledge of the orbital and stellar parameters of HD 54662 and to …

2018 Astronomy and Astrophysics
XMM-Newton 8
THROES: a caTalogue of HeRschel Observations of Evolved Stars. I. PACS range spectroscopy
DOI: 10.1051/0004-6361/201731940 Bibcode: 2018A&A...611A..41R

García-Lario, P.; Solano, E.; Sánchez Contreras, C. +3 more

This is the first of a series of papers presenting the THROES (A caTalogue of HeRschel Observations of Evolved Stars) project, intended to provide a comprehensive overview of the spectroscopic results obtained in the far-infrared (55-670 µm) with the Herschel space observatory on low-to-intermediate mass evolved stars in our Galaxy. Here we …

2018 Astronomy and Astrophysics
AKARI Herschel ISO 8
LBT/ARGOS adaptive optics observations of z ∼ 2 lensed galaxies
DOI: 10.1051/0004-6361/201732387 Bibcode: 2018A&A...618A..36P

Lutz, D.; Grillo, C.; Contursi, A. +24 more


Aims: Gravitationally lensed systems allow a detailed view of galaxies at high redshift. High spatial- and spectral-resolution measurements of arc-like structures can offer unique constraints on the physical and dynamical properties of high-z systems.
Methods: We present near-infrared spectra centred on the gravitational arcs of six know…

2018 Astronomy and Astrophysics
eHST 8
Long-term variations in the X-ray activity of HR 1099
DOI: 10.1051/0004-6361/201732222 Bibcode: 2018A&A...616A.161P

Schmitt, J. H. M. M.; Robrade, J.; Schneider, P. C. +6 more

Context. Although timing variations in close binary systems have been studied for a long time, their underlying causes are still unclear. A possible explanation is the so-called Applegate mechanism, where a strong, variable magnetic field can periodically change the gravitational quadrupole moment of a stellar component, thus causing observable pe…

2018 Astronomy and Astrophysics
Exosat XMM-Newton 8
Star formation history of Canis Major OB1. II. A bimodal X-ray population revealed by XMM-Newton
DOI: 10.1051/0004-6361/201730815 Bibcode: 2018A&A...609A.127S

Montmerle, T.; Stelzer, B.; Gregorio-Hetem, J. +2 more


Aims: The Canis Major OB1 Association has an intriguing scenario of star formation, especially in the region called Canis Major R1 (CMa R1) traditionally assigned to a reflection nebula, but in reality an ionized region. This work is focussed on the young stellar population associated with CMa R1, for which our previous results from ROSAT, op…

2018 Astronomy and Astrophysics
XMM-Newton 8
The VMC Survey. XXXII. Pre-main-sequence populations in the Large Magellanic Cloud
DOI: 10.1051/0004-6361/201833951 Bibcode: 2018A&A...620A.143Z

Sun, Ning-Chen; de Grijs, Richard; Marconi, Marcella +11 more

Context. Detailed studies of intermediate- and low-mass pre-main-sequence (PMS) stars outside the Galaxy have so far been conducted only for small targeted regions harbouring known star formation complexes. The VISTA Survey of the Magellanic Clouds (VMC) provides an opportunity to study PMS populations down to solar masses on a galaxy-wide scale. …

2018 Astronomy and Astrophysics
Herschel eHST 8