Search Publications

Expanding hot flow in the black hole binary SWIFT J1753.5-0127: evidence from optical timing
DOI: 10.1093/mnras/stx1207 Bibcode: 2017MNRAS.470...48V

Gandhi, Poshak; Tsygankov, Sergey S.; Poutanen, Juri +5 more

We describe the evolution of optical and X-ray temporal characteristics during the outburst decline of the black hole X-ray binary SWIFT J1753.5-0127. The optical/X-ray cross-correlation function demonstrates a single positive correlation at the outburst peak, then it has multiple dips and peaks during the decline stage, which are then replaced by…

2017 Monthly Notices of the Royal Astronomical Society
INTEGRAL 25
Detection of an ∼20 kpc coherent magnetic field in the outskirt of merging spirals: the Antennae galaxies
DOI: 10.1093/mnras/stw2369 Bibcode: 2017MNRAS.464.1003B

Mao, S. A.; Zweibel, Ellen G.; Basu, Aritra +3 more

We present a study of the magnetic field properties of NGC 4038/9 (the `Antennae' galaxies), the closest example of a late stage merger of two spiral galaxies. Wideband polarimetric observations were performed using the Karl G. Jansky Very Large Array between 2 and 4 GHz. Rotation measure synthesis and Faraday depolarization analysis was performed…

2017 Monthly Notices of the Royal Astronomical Society
eHST 25
Dwarf spheroidal J-factors without priors: A likelihood-based analysis for indirect dark matter searches
DOI: 10.1093/mnras/stw3079 Bibcode: 2017MNRAS.466..669C

Cohen-Tanugi, J.; Conrad, J.; Anderson, B. +3 more

Line-of-sight integrals of the squared density, commonly called the J-factor, are essential for inferring dark matter (DM) annihilation signals. The J-factors of DM-dominated dwarf spheroidal satellite galaxies (dSphs) have typically been derived using Bayesian techniques, which for small data samples implies that a choice of priors constitutes a …

2017 Monthly Notices of the Royal Astronomical Society
Gaia 25
High-resolution spectroscopy of the extended narrow-line region of IC 5063 and NGC 7212
DOI: 10.1093/mnras/stx1628 Bibcode: 2017MNRAS.471..562C

La Mura, G.; Ciroi, S.; Cracco, V. +6 more

We studied the properties of the gas of the extended narrow-line region (ENLR) of two Seyfert 2 galaxies: IC 5063 and NGC 7212. We analysed high-resolution spectra to investigate how the main properties of this region depend on the gas velocity. We divided the emission lines in velocity bins and we calculated several line ratios. Diagnostic diagra…

2017 Monthly Notices of the Royal Astronomical Society
eHST 25
The Hubble Space Telescope UV Legacy Survey of Galactic globular clusters - XI. The horizontal branch in NGC 6388 and NGC 6441
DOI: 10.1093/mnras/stw2790 Bibcode: 2017MNRAS.465.1046T

Salaris, M.; Di Criscienzo, M.; Anderson, J. +12 more

The Hubble Space Telescope UV Legacy survey of Galactic globular clusters (GC) is characterizing many different aspects of their multiple stellar populations. The `Grundahl-jump' (G-jump) is a discontinuity in ultraviolet brightness of blue horizontal branch (HB) stars, signalling the onset of radiative metal levitation. The HB Legacy data confirm…

2017 Monthly Notices of the Royal Astronomical Society
eHST 25
Kinematics of Subluminous O and B Stars by Surface Helium Abundance
DOI: 10.1093/mnras/stw3305 Bibcode: 2017MNRAS.467...68M

Jeffery, C. S.; Woolf, V. M.; Martin, P. +1 more

The majority of hot subdwarf stars are low-mass core-helium-burning stars. Their atmospheres are generally helium deficient; however, a minority have extremely helium-rich surfaces. An additional fraction have an intermediate surface-helium abundance, occasionally accompanied by peculiar abundances of other elements. We have identified a sample of…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 25
HST and ground-based spectroscopy of quasar outflows: from mini-BALs to BALs
DOI: 10.1093/mnras/stx775 Bibcode: 2017MNRAS.468.4539M

Shields, J. C.; Hamann, F.; Capellupo, D. M. +3 more

Quasar outflows have been posited as a mechanism to couple supermassive black holes to evolution in their host galaxies. We use multi-epoch spectra from the Hubble Space Telescope (HST) and ground-based observatories to study the outflows in seven quasars that have C IV outflow lines ranging from a classic broad absorption line (BAL) to weaker/nar…

2017 Monthly Notices of the Royal Astronomical Society
eHST 25
Photometric behaviour of 67P/Churyumov-Gerasimenko and analysis of its pre-perihelion diurnal variations
DOI: 10.1093/mnras/stx1803 Bibcode: 2017MNRAS.469S.346L

Mottola, S.; Erard, S.; Capaccioni, F. +14 more

Spectral parameters measured by the Rosetta/VIRTIS imaging spectrometer on the nucleus of comet 67P/Churyumov-Gerasimenko were studied as a function of incidence, emission and phase angles. A statistical analysis was undertaken for a number of spectral parameters: reflectance at seven wavelengths (0.55, 0.75, 1.2, 1.7, 2.0, 2.8 and 4.0 µm), …

2017 Monthly Notices of the Royal Astronomical Society
Rosetta 25
A strongly truncated inner accretion disc in the Rapid Burster
DOI: 10.1093/mnrasl/slw244 Bibcode: 2017MNRAS.466L..98V

Degenaar, N.; Fabian, A. C.; van den Eijnden, J. +4 more

The neutron star (NS) low-mass X-ray binary (LMXB) the Rapid Burster (RB; MXB 1730-335) uniquely shows both Type I and Type II X-ray bursts. The origin of the latter is ill-understood but has been linked to magnetospheric gating of the accretion flow. We present a spectral analysis of simultaneous Swift, NuSTAR and XMM-Newton observations of the R…

2017 Monthly Notices of the Royal Astronomical Society
XMM-Newton 25
Weighing in on the masses of retired A stars with asteroseismology: K2 observations of the exoplanet-host star HD 212771
DOI: 10.1093/mnras/stx876 Bibcode: 2017MNRAS.469.1360C

Vanderburg, Andrew; Chaplin, William J.; Davies, Guy R. +12 more

Doppler-based planet surveys point to an increasing occurrence rate of giant planets with stellar mass. Such surveys rely on evolved stars for a sample of intermediate-mass stars (so-called retired A stars), which are more amenable to Doppler observations than their main-sequence progenitors. However, it has been hypothesized that the masses of su…

2017 Monthly Notices of the Royal Astronomical Society
Gaia 25