Search Results - "PONTI, G"
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Detection of large-scale X-ray bubbles in the Milky Way halo
Published in Nature (London) (10-12-2020)“…The halo of the Milky Way provides a laboratory to study the properties of the shocked hot gas that is predicted by models of galaxy formation. There is…”
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2
Discovery of a relation between black hole mass and soft X-ray time lags in active galactic nuclei
Published in Monthly notices of the Royal Astronomical Society (21-05-2013)“…We carried out a systematic analysis of time lags between X-ray energy bands in a large sample (32 sources) of unabsorbed, radio quiet active galactic nuclei…”
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3
Not that long time ago in the nearest galaxy: 3D slice of molecular gas revealed by a 110 yr old flare of Sgr A
Published in Monthly notices of the Royal Astronomical Society (11-02-2017)“…A powerful outburst of X-ray radiation from the supermassive black hole Sgr A* at the centre of the Milky Way is believed to be responsible for the…”
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4
Regulation of black-hole accretion by a disk wind during a violent outburst of V404 Cygni
Published in Nature (London) (02-06-2016)“…A sustained, neutral wind from the outer accretion disk is observed in the transient black hole V404 Cygni during a violent outburst; this unusual wind, which…”
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5
A tidal disruption flare in a massive galaxy? Implications for the fuelling mechanisms of nuclear black holes
Published in Monthly notices of the Royal Astronomical Society (01-09-2015)“…We argue that the ‘changing look’ active galactic nucleus (AGN) recently reported by LaMassa et al. could be a luminous flare produced by the tidal disruption…”
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6
An X-ray chimney extending hundreds of parsecs above and below the Galactic Centre
Published in Nature (London) (01-03-2019)“…Evidence has mounted in recent decades that outflows of matter and energy from the central few parsecs of our Galaxy have shaped the observed structure of the…”
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7
Ubiquitous equatorial accretion disc winds in black hole soft states
Published in Monthly notices of the Royal Astronomical Society. Letters (01-05-2012)“…ABSTRACT High‐resolution spectra of Galactic black holes (GBHs) reveal the presence of highly ionized absorbers. In one GBH, accreting close to the Eddington…”
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8
X-ray Quasi-Periodic Eruptions from Two Previously Quiescent Galaxies
Published in Nature (London) (29-04-2021)“…Quasi-Periodic Eruptions (QPEs) are extreme high-amplitude bursts of X-ray radiation recurring every few hours and originating near the central supermassive…”
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9
X-Ray Observations of the Isolated Black Hole Candidate OGLE-2011-BLG-0462 and Other Collapsed Objects Discovered through Gravitational Microlensing
Published in The Astrophysical journal (01-07-2022)“…Abstract Isolated black holes and neutron stars can be revealed through the observation of long-duration gravitational microlensing events. A few candidates…”
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10
Relativistic Fe Kα line study in Seyfert 1 galaxies observed with Suzaku
Published in Monthly notices of the Royal Astronomical Society (01-06-2016)“…We present an analysis of a sample of Seyfert 1 galaxies observed with Suzaku. The aim of this work is to examine critically the evidence for a relativistic Fe…”
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11
Revealing accretion on to black holes: X-ray reflection throughout three outbursts of GX 339−4
Published in Monthly notices of the Royal Astronomical Society (01-08-2014)“…Understanding the dynamics behind black hole state transitions and the changes they reflect in outbursts has become long-standing problem. The X-ray reflection…”
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12
Discovery of a Superluminal Fe K Echo at the Galactic Center: The Glorious Past of Sgr A Preserved by Molecular Clouds
Published in The Astrophysical journal (01-05-2010)“…We present the result of a study of the X-ray emission from the galactic center (GC) molecular clouds (MCs) within 15 arcmin from Sgr A*. We use XMM-Newton…”
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High-energy monitoring of NGC 4593 II. Broad-band spectral analysis: testing the two-corona model
Published in Monthly notices of the Royal Astronomical Society (11-03-2019)“…It is widely believed that the primary X-ray emission of AGN is due to the Comptonization of optical-UV photons from a hot electron corona, while the origin of…”
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14
Simultaneous X-Ray and Infrared Observations of Sagittarius A's Variability
Published in The Astrophysical journal (01-02-2019)“…Emission from Saggitarius A* is highly variable at both X-ray and infrared (IR) wavelengths. Observations over the last ∼20 yr have revealed X-ray flares that…”
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15
The XMM–Newton view of the central degrees of the Milky Way
Published in Monthly notices of the Royal Astronomical Society (11-10-2015)“…The deepest XMM–Newton mosaic map of the central 1 $_{.}^{\circ}$ 5 of the Galaxy is presented, including a total of about 1.5 Ms of EPIC-pn cleaned exposures…”
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16
Inclination and relativistic effects in the outburst evolution of black hole transients
Published in Monthly notices of the Royal Astronomical Society (21-06-2013)“…We have systematically studied the effect of the orbital inclination in the outburst evolution of black hole transients. We have included all the systems…”
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A powerful flare from Sgr A confirms the synchrotron nature of the X-ray emission
Published in Monthly notices of the Royal Astronomical Society (01-06-2017)“…Abstract We present the first fully simultaneous fits to the near-infrared (NIR) and X-ray spectral slope (and its evolution) during a very bright flare from…”
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18
Broad line emission from iron K- and L-shell transitions in the active galaxy 1H 0707-495
Published in Nature (28-05-2009)“…Since the 1995 discovery of the broad iron K-line emission from the Seyfert galaxy MCG-6-30-15 (ref. 1), broad iron K lines have been found in emission from…”
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The puzzling orbital period evolution of the LMXB AX J1745.6−2901
Published in Monthly notices of the Royal Astronomical Society (01-01-2017)“…The orbital period evolution of X-ray binaries provides fundamental clues to understanding mechanisms of angular momentum transfer and loss in these systems…”
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Long XMM observation of the narrow-line Seyfert 1 galaxy IRAS 13224−3809: rapid variability, high spin and a soft lag
Published in Monthly notices of the Royal Astronomical Society (11-03-2013)“…The narrow-line Seyfert 1 galaxy IRAS 13224−3809 has been observed with XMM-Newton for 500 ks. The source is rapidly variable on time-scales down to a few 100…”
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