Zobrazeno 1 - 10
of 27
pro vyhledávání: '"D Lawther"'
Publikováno v:
Lawther, D, Vestergaard, M, Raimundo, S, Koay, J Y, Peterson, B M, Fan, X, Grupe, D & Mathur, S 2023, ' Flares in the changing look AGN Mrk 590-I. The UV response to X-ray outbursts suggests a more complex reprocessing geometry than a standard disc ', Monthly Notices of the Royal Astronomical Society, vol. 519, no. 3, pp. 3903-3922 . https://doi.org/10.1093/mnras/stac3515
Mrk 590 is a known changing-look AGN which almost turned off in 2012, and then in 2017 partially re-ignited into a repeat flaring state, unusual for an AGN. Our \emph{Swift} observations since 2013 allow us to characterise the accretion-generated emi
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 467:4674-4710
We present the Swift optical to X-ray spectral energy distributions (SEDs) of 44 quasars at redshifts z~2 observed by Swift, part of a larger program to establish and characterize the optical through X-ray SEDs of moderate-redshift quasars. Here we o
Publikováno v:
Raimundo, S I, Vestergaard, M, Koay, J Y, Lawther, D, Casasola, V & Peterson, B M 2019, ' MUSE observations of a changing-look AGN I : The re-appearance of the broad emission lines ', Monthly Notices of the Royal Astronomical Society, vol. 486, no. 1, pp. 123-140 . https://doi.org/10.1093/mnras/stz852
Optical changing-look Active Galactic Nuclei (AGN) are a class of sources that change type within a short timescale of years or decades. This change is characterised by the appearance or disappearance of broad emission lines, often associated with dr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e9af59a2b0ff678c8205f581cf56df84
http://arxiv.org/abs/1903.08696
http://arxiv.org/abs/1903.08696
Disk reverberation mapping of a handful of nearby AGN suggest accretion disk sizes which are a factor few too large for their luminosities, apparently at odds with the standard model. Here, we investigate the likely contribution to the measured delay
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d5849335c09cb605be34bca5a60fd3ba
We study the host galaxies of four Iron Low-Ionization Broad Absorption-line Quasars (FeLoBALs) using Hubble Space Telescope imaging data, investigating the possibility that they represent a transition between an obscured AGN and an ordinary optical
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2cb3c9cd3da7bf2900b2998f43d198ff
http://arxiv.org/abs/1712.04403
http://arxiv.org/abs/1712.04403
Akademický článek
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We investigate if the active galactic nucleus (AGN) of Mrk 590, whose supermassive black hole was until recently highly accreting, is turning off due to a lack of central gas to fuel it. We analyse new sub-arcsecond resolution ALMA maps of the $^{12}
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::14130b08600232f25303551e497d3724
http://arxiv.org/abs/1509.09203
http://arxiv.org/abs/1509.09203
Publikováno v:
Proceedings of the International Astronomical Union. 11
FeLoBAL quasars may be an early evolutionary stage of merger-triggered quasar activity. We test this hypothesis using HST imaging of four FeLoBAL quasars. The host galaxy colors are consistent with early-type quiescent galaxies or heavily-obscured st
Autor:
John D. Lawther
Publikováno v:
Educational psychology.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::ac5b33cb7ca5c06fb43f34b0e804631f
https://doi.org/10.1037/13511-003
https://doi.org/10.1037/13511-003
Publikováno v:
Lawther, D P, Paarup, T, Schmidt, M, Vestergaard, M, Hjorth, J & Malesani, D 2012, ' Constraints on the relative sizes of intervening Mg II-absorbing clouds and quasar emitting regions ', Astronomy & Astrophysics, vol. 546, A67 . https://doi.org/10.1051/0004-6361/201219326
Context: A significantly higher incidence of strong (rest equivalent width W_r > 1 {\AA}) intervening Mg II absorption is observed along gamma-ray burst (GRB) sight-lines relative to those of quasar sight-lines. A geometrical explanation for this dis