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H.E.S.S. and Suzaku observations of the Vela X pulsar wind nebula
DOI: 10.1051/0004-6361/201935458 Bibcode: 2019A&A...627A.100H

Santangelo, A.; Quirrenbach, A.; Bregeon, J. +222 more

Context. Pulsar wind nebulae (PWNe) represent the most prominent population of Galactic very-high-energy gamma-ray sources and are thought to be an efficient source of leptonic cosmic rays. Vela X is a nearby middle-aged PWN, which shows bright X-ray and TeV gamma-ray emission towards an elongated structure called the cocoon.
Aims: Since TeV …

2019 Astronomy and Astrophysics
Suzaku 16
Variations on a theme: the puzzling behaviour of Schulte 12
DOI: 10.1051/0004-6361/201935141 Bibcode: 2019A&A...627A..99N

Nazé, Yaël; Mahy, Laurent; Rauw, Gregor +2 more

One of the first massive stars detected in X-rays, Schulte 12 has remained a puzzle in several aspects. In particular, its extreme brightness both in the visible and X-ray ranges is intriguing. Thanks to Swift and XMM-Newton observations covering ∼5000 d, we report the discovery of a regular 108 d modulation in X-ray flux of unknown origin. The mi…

2019 Astronomy and Astrophysics
Gaia INTEGRAL Suzaku XMM-Newton 11
Spectral analysis of the dipping LMXB system XB 1916-053
DOI: 10.1051/0004-6361/201832984 Bibcode: 2019A&A...625A..92G

Sanna, A.; Di Salvo, T.; Burderi, L. +6 more

Context. XB 1916-053 is a low mass X-ray binary system (LMXB) hosting a neutron star (NS) and showing periodic dips. The spectrum of the persistent emission was modeled with a blackbody component having a temperature between 1.31 and 1.67 keV and with a Comptonization component with an electron temperature of 9.4 keV and a photon index Γ between 2…

2019 Astronomy and Astrophysics
Suzaku 10