Search Publications

Revealing the nature of central emission nebulae in the dwarf galaxy NGC 185
DOI: 10.1051/0004-6361/201935818 Bibcode: 2019A&A...628A..87V

Ilić, D.; Vučetić, M. M.; Onić, D. +6 more


Aims: In this paper we present new optical observations of the galaxy NGC 185 intended to reveal the status of supernova remnants (SNRs) in this dwarf companion of the Andromeda galaxy. Previously, it was reported that this galaxy hosts one SNR.
Methods: Our deep photometric study with the 2m telescope at Rozhen National Astronomical Obs…

2019 Astronomy and Astrophysics
XMM-Newton 3
Murchison Widefield Array and XMM-Newton observations of the Galactic supernova remnant G5.9+3.1
DOI: 10.1051/0004-6361/201834230 Bibcode: 2019A&A...625A..93O

Haberl, F.; Callingham, J. R.; Filipović, M. D. +27 more


Aims: In this paper we discuss the radio continuum and X-ray properties of the so-far poorly studied Galactic supernova remnant (SNR) G5.9 + 3.1.
Methods: We present the radio spectral energy distribution (SED) of the Galactic SNR G5.9 + 3.1 obtained with the Murchison Widefield Array (MWA). Combining these new observations with the surv…

2019 Astronomy and Astrophysics
XMM-Newton 3
Link between trees of fragmenting granules and deep downflows in MHD simulation
DOI: 10.1051/0004-6361/201834283 Bibcode: 2019A&A...622A.112R

Malherbe, J. M.; Roudier, T.; Frank, Z. +1 more

Context. Trees of fragmenting granules (TFG) and associated flows are suspected to play a major role in the formation of the network in the quiet Sun. We investigate the counterparts, in terms of dynamics, of surface structures detectable by high resolution observations in deeper layers up to 15 Mm, which are only available from numerical simulati…

2019 Astronomy and Astrophysics
Hinode SOHO 3
Absolute dimensions of the low-mass eclipsing binary system NSVS 10653195
DOI: 10.1051/0004-6361/201935516 Bibcode: 2019A&A...627A.153I

Torres, Guillermo; López-Morales, Mercedes; Coughlin, Jeffrey L. +3 more

Context. Low-mass stars in eclipsing binary systems show radii larger and effective temperatures lower than theoretical stellar models predict for isolated stars with the same masses. Eclipsing binaries with low-mass components are hard to find due to their low luminosity. As a consequence, the analysis of the known low-mass eclipsing systems is k…

2019 Astronomy and Astrophysics
Gaia 3
X-ray analysis of the accreting supermassive black hole in the radio galaxy PKS 2251+11
DOI: 10.1051/0004-6361/201935176 Bibcode: 2019A&A...625A..26R

Tombesi, F.; Panessa, F.; Bruni, G. +2 more

Context. We have investigated the dichotomy between jetted and non-jetted active galactic nuclei (AGNs), focusing on the fundamental differences of these two classes in the accretion physics onto the central supermassive black hole (SMBH). We tested the validity of the unification model of AGNs through the characterization of the mutual interactio…

2019 Astronomy and Astrophysics
XMM-Newton 3
UV core dimming in coronal streamer belt and the projection effects
DOI: 10.1051/0004-6361/201834299 Bibcode: 2019A&A...623A..95A

Abbo, L.; Giordano, S.; Ofman, L.

During solar minimum activity, the coronal structure is dominated by a tilted streamer belt, associated with the sources of the slow solar wind. It is known that some UV coronal spectral observations show a quite evident core dimming in heavy ions emission in quiescent streamers. In this paper, our purpose is to investigate this phenomenon by comp…

2019 Astronomy and Astrophysics
SOHO 3
Open cluster kinematics with Gaia DR2 (Corrigendum)
DOI: 10.1051/0004-6361/201834020e Bibcode: 2019A&A...623C...2S

Castro-Ginard, A.; Jordi, C.; Casamiquela, L. +16 more

The table with clusters velocities is only available at the CDS via anonymous ftp to http://cdsarc.u-strasbg.fr (http://130.79.128.5) or via http://cdsarc.u-strasbg.fr/viz-bin/qcat?J/A+A/623/C2

2019 Astronomy and Astrophysics
Gaia 3
Ultraviolet photo-ionisation in far-infrared selected sources
DOI: 10.1051/0004-6361/201935827 Bibcode: 2019A&A...627A..93C

Curran, S. J.; Duchesne, S. W.

It has been reported that there is a deficit of stellar heated dust, as evident from the lack of far-infrared (FIR) emission, in sources within the Herschel-SPIRE sample with X-ray luminosities exceeding a critical value of LX ∼ 1037 W. Such a scenario would be consistent with the suppression of star formation by the AGN, req…

2019 Astronomy and Astrophysics
Herschel 3
Comparative analysis of solar radio bursts before and during CME propagation
DOI: 10.1051/0004-6361/201629489 Bibcode: 2019A&A...625A..63D

Poedts, S.; Dididze, G.; Shergelashvili, B. M. +5 more

Context. As is well known, coronal mass ejection (CME) propagation often results in the fragmentation of the solar atmosphere on smaller regions of density (magnetic field) enhancement (depletion). It is expected that this type of fragmentation may have radio signatures.
Aims: The general aim of the present paper is to perform a comparative a…

2019 Astronomy and Astrophysics
SOHO 3
Joint cluster reconstructions. Combing free-form lensing and X-rays
DOI: 10.1051/0004-6361/201834928 Bibcode: 2019A&A...627A.143H

Bartelmann, Matthias; Merten, Julian; Hilbert, Stefan +2 more

Context. Galaxy clusters provide a multitude of observational data across wavelengths, and their structure and morphology are of considerable interest in cosmology as well as astrophysics.
Aims: We develop a framework that allows the combination of lensing and non-lensing observations in a free-form and mesh-free approach to infer the project…

2019 Astronomy and Astrophysics
XMM-Newton 3