Search Publications

A Changing-Look AGN to Be Probed by X-ray Polarimetry
DOI: 10.3390/galaxies6020052 Bibcode: 2018Galax...6...52A

Miniutti, Giovanni; Agís-González, Beatriz; Hutsemékers, Damien

Active galactic nuclei (AGN) produce the highest intrinsic luminosities in the Universe from within a compact region. The central engine is thought to be powered by accretion onto a supermassive black hole. A fraction of this huge release of energy influences the evolution of the host galaxy, and in particular, star formation. Thus, AGN are key as…

2018 Galaxies
XMM-Newton 2
Analysis of a Failed Eclipse Plasma Ejection Using EUV Observations
DOI: 10.1007/s11207-018-1257-x Bibcode: 2018SoPh..293...42T

Koutchmy, S.; Tavabi, E.; Bazin, C.

The photometry of eclipse white-light (W-L) images showing a moving blob is interpreted for the first time together with observations from space with the PRoject for On Board Autonomy (PROBA-2) mission (ESA). An off-limb event seen with great details in W-L was analyzed with the SWAP imager (Sun Watcher using Active pixel system detector and image…

2018 Solar Physics
PROBA-2 SOHO 2
A unique distant submillimeter galaxy with an X-ray-obscured radio-luminous active galactic nucleus
DOI: 10.1051/0004-6361/201833434 Bibcode: 2018A&A...619A..76S

Daddi, E.; Elbaz, D.; Wang, T. +10 more


Aims: We present a multiwavelength study of an atypical submillimeter galaxy, GH500.30, in the GOODS-North field, with the aim to understand its physical properties of stellar and dust emission, as well as the central active galactic nucleus (AGN) activity. Although it is shown that the source is likely an extremely dusty galaxy at high redsh…

2018 Astronomy and Astrophysics
eHST 2
EXTraS discovery of a peculiar flaring X-ray source in the Galactic globular cluster NGC 6540
DOI: 10.1051/0004-6361/201833086 Bibcode: 2018A&A...616A..36M

Mereghetti, Sandro; Tiengo, Andrea; Belfiore, Andrea +7 more

We report the discovery of a flaring X-ray source 7″ from the center of the globular cluster NGC 6540 obtained during the EXTraS project devoted to a systematic search for variability in archival data of the XMM-Newton satellite. The source had a quiescent X-ray luminosity on the order of 1032 erg s-1 in the 0.5-10 keV range …

2018 Astronomy and Astrophysics
XMM-Newton eHST 2
Limits on the Contribution of Endogenic Radiolysis to the Presence of Molecular Oxygen in Comet 67P/Churyumov-Gerasimenko
DOI: 10.3847/1538-4357/aad22f Bibcode: 2018ApJ...864....9B

Mousis, Olivier; Bouquet, Alexis; Nicolaou, Georgios +6 more

Radiolytic production has been proposed as a potential source for the molecular oxygen observed in comet 67P/Churyumov-Gerasimenko. Radiolysis can be exogenic or endogenic, the latter due to radionuclides present in the dust constitutive of the comet nucleus. We investigated the possibility of forming a significant amount of molecular oxygen throu…

2018 The Astrophysical Journal
Rosetta 2
In-Orbit Performance of the Digital Electronics for the X-Ray Microcalorimeter Onboard the Hitomi Satellite
DOI: 10.1007/s10909-018-1861-z Bibcode: 2018JLTP..193..505T

Tsujimoto, M.; Tashiro, M. S.; Ishisaki, Y. +9 more

The pulse shape processor is the onboard digital electronics unit of the X-ray microcalorimeter instrument—the soft X-ray spectrometer—onboard the Hitomi satellite. It processes X-ray events using the optimum filtering with limited resources. It was operated for 36 days in orbit continuously without issues and met the requirement of processing a 1…

2018 Journal of Low Temperature Physics
Hitomi 2
Variable interstellar absorption lines in young stellar aggregates
DOI: 10.1093/mnras/sty531 Bibcode: 2018MNRAS.476.4987K

Krełowski, J.; Strobel, A.; Vješnica, S. +2 more

The variability of interstellar atomic lines, sporadically reported in the astronomical literature, has been confirmed both in the case of the nearby hot star δ Ori and the very young and violent star-forming region η Carinae, using high-resolution echelle spectra. The presented variability concerns the intensities and profiles of Na I, K I and Ca…

2018 Monthly Notices of the Royal Astronomical Society
Gaia 2
Warm CO in evolved stars from the THROES catalogue. I. Herschel-PACS spectroscopy of O-rich envelopes (Corrigendum)
DOI: 10.1051/0004-6361/201833177e Bibcode: 2018A&A...619C...2R

García-Lario, P.; Sánchez Contreras, C.; da Silva Santos, J. M. +1 more

2018 Astronomy and Astrophysics
Herschel 2
Optimizing asteroid orbit computation for Gaia with normal points
DOI: 10.1051/0004-6361/201833197 Bibcode: 2018A&A...620A.101F

Muinonen, Karri; Fedorets, Grigori; Granvik, Mikael +11 more

Context. In addition to the systematic observations of known solar-system objects (SSOs), a continuous processing of new discoveries requiring fast responses is implemented as the short-term processing of Gaia SSO observations, providing alerts for ground-based follow-up observers. The common independent observation approach for the purposes of or…

2018 Astronomy and Astrophysics
Gaia 2
Infrared Photometric Study of Wolf-Rayet Galaxies
DOI: 10.3847/1538-3881/aa988c Bibcode: 2018AJ....155...17C

Chen, P. S.; Yang, X. H.; Liu, J. Y. +1 more

We collected observational data on 781 Wolf-Rayet (WR) galaxies from the literature to photometrically study their infrared properties measured by the 2MASS, WISE, IRAS, AKARI, and Herschel missions. It is found that in the 1-5 µm range the radiations of WR galaxies are dominated by the free-free emissions from the stellar winds and the circ…

2018 The Astronomical Journal
AKARI Herschel 2