Search Publications

LOFAR observations of decameter carbon radio recombination lines towards Cassiopeia A
DOI: 10.1093/mnras/stx239 Bibcode: 2017MNRAS.467.2274S

van Weeren, R. J.; Tielens, A. G. G. M.; Röttgering, H. J. A. +6 more

We present a study of carbon radio recombination lines towards Cassiopeia A using low frequency array (LOFAR) observations in the frequency range 10-33 MHz. Individual carbon α lines are detected in absorption against the continuum at frequencies as low as 16 MHz. Stacking several Cα lines we obtain detections in the 11-16 MHz range. These are the…

2017 Monthly Notices of the Royal Astronomical Society
Herschel 26
Constraints on AGN feedback from its Sunyaev-Zel'dovich imprint on the cosmic background radiation
DOI: 10.1093/mnras/stx492 Bibcode: 2017MNRAS.468..577S

Sijacki, Debora; Efstathiou, George; Puchwein, Ewald +2 more

We derive constraints on feedback by active galactic nuclei (AGN) by setting limits on their thermal Sunyaev-Zel'dovich (SZ) imprint on the cosmic microwave background. The amplitude of any SZ signature is small and degenerate with the poorly known sub-mm spectral energy distribution of the AGN host galaxy and other unresolved dusty sources along …

2017 Monthly Notices of the Royal Astronomical Society
AKARI Planck 26
Discovery of a glitch in the accretion-powered pulsar SXP 1062
DOI: 10.1093/mnras/stx1771 Bibcode: 2017MNRAS.471.4982S

Serim, M. M.; Şahiner, Ş.; ćerri-Serim, D. +2 more

We present timing analysis of the accretion-powered pulsar SXP 1062, based on the observations of Swift, XMM-Newton and Chandra satellites covering a time span of about 2 yr. We obtain a phase coherent timing solution that shows that SXP 1062 has been steadily spinning down with a rate -4.29(7) × 10-14 Hz s-1 leading to a sur…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 26
Long-term survival of surface water ice on comet 67P
DOI: 10.1093/mnras/stx2298 Bibcode: 2017MNRAS.469S.582O

Jorda, L.; Lamy, P. L.; Lara, L. M. +53 more

Numerous water-ice-rich deposits surviving more than several months on comet 67P/Churyumov-Gerasimenko were observed during the Rosetta mission. We announce the first-time detection of water-ice features surviving up to 2 yr since their first observation via OSIRIS (Optical, Spectroscopic, and Infrared Remote Imaging System) NAC (narrow angle came…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 26
Obscured active galactic nuclei triggered in compact star-forming galaxies
DOI: 10.1093/mnrasl/slw247 Bibcode: 2017MNRAS.466L.103C

Juneau, Stéphanie; Capak, Peter; McCracken, H. J. +10 more

We present a structural study of 182 obscured active galactic nuclei (AGNs) at z ≤ 1.5, selected in the Cosmic Evolution Survey field from their extreme infrared to X-ray luminosity ratio and their negligible emission at optical wavelengths. We fit optical to far-infrared spectral energy distributions and analyse deep Hubble Space Telescope imagin…

2017 Monthly Notices of the Royal Astronomical Society
eHST 26
The puzzling orbital period evolution of the LMXB AX J1745.6-2901
DOI: 10.1093/mnras/stw2317 Bibcode: 2017MNRAS.464..840P

Stella, L.; Nandra, K.; Ponti, G. +2 more

The orbital period evolution of X-ray binaries provides fundamental clues to understanding mechanisms of angular momentum transfer and loss in these systems. We present an X-ray eclipse timing analysis of the transient low-mass X-ray binary AX J1745.6-2901. This system shows full eclipses and thus is one of the few objects of this class for which …

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 26
Lower hybrid waves at comet 67P/Churyumov-Gerasimenko
DOI: 10.1093/mnras/stx868 Bibcode: 2017MNRAS.469S..29A

André, M.; Karlsson, T.; Henri, P. +9 more

We investigate the generation of waves in the lower hybrid frequency range by density gradients in the near plasma environment of comet 67P/Churyumov-Gerasimenko. When the plasma is dominated by water ions from the comet, a situation with magnetized electrons and unmagnetized ions is favourable for the generation of lower hybrid waves. These waves…

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 26
Revisiting the extremely fast disc wind in a gravitationally lensed quasar APM 08279+5255
DOI: 10.1093/mnras/stx559 Bibcode: 2017MNRAS.468.1442H

Done, Chris; Takahashi, Tadayuki; Hagino, Kouichi +2 more

The gravitationally lensed quasar APM 08279+5255 has the fastest claimed wind from any active galactic nucleus, with velocities of 0.6-0.7c, requiring magnetic acceleration as special relativistic effects limit all radiatively driven winds to v < 0.3-0.5c. However, this extreme velocity derives from interpreting both the narrow and broad absorp…

2017 Monthly Notices of the Royal Astronomical Society
AKARI XMM-Newton 26
A close encounter of the massive kind
DOI: 10.1093/mnras/stw2618 Bibcode: 2017MNRAS.464.3561M

Maíz Apellániz, J.; Sana, H.; Barbá, R. H. +2 more

We have used (I) Hubble Space Telescope Advanced Camera for Surveys imaging and Space Telescope Imaging Spectrograph spectroscopy, (II) ground-based Precision Integrated-Optics Near-infrared Imaging ExpeRiment/Very Large Telescope long-baseline interferometry, and (III) ground-based spectroscopy from different instruments to study the orbit of the…

2017 Monthly Notices of the Royal Astronomical Society
eHST 25
Outbursts of the intermediate-mass black hole HLX-1: a wind-instability scenario
DOI: 10.1093/mnras/stx888 Bibcode: 2017MNRAS.469..886S

Soria, Roberto; Wu, Kinwah; Zampieri, Luca +5 more

We model the intermediate-mass black hole HLX-1, using the Hubble Space Telescope, XMM-Newton and Swift. We quantify the relative contributions of a bluer component, function of X-ray irradiation, and a redder component, constant and likely coming from an old stellar population. We estimate a black hole mass {≈ } (2^{+2}_{-1}) × 10^4 M_{⊙}, a spin…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton eHST 25