Zobrazeno 1 - 10
of 24
pro vyhledávání: '"Daniel M. Capellupo"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 475:585-600
Quasar outflows have long been recognized as potential contributors to the co-evolution between supermassive black holes (SMBHs) and their host galaxies. The role of outflows in AGN feedback processes can be better understood by placing observational
Autor:
Emily Moravec, Fred Hamann, P. Rodriguez Hidalgo, Daniel M. Capellupo, Joseph C. Shields, S. M. McGraw
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 468:4539-4555
Quasar outflows have been posited as a mechanism to couple super-massive black holes to evolution in their host galaxies. We use multi-epoch spectra from the Hubble Space Telescope and ground-based observatories to study the outflows in seven quasars
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2019, 483, pp.1808-1828. ⟨10.1093/mnras/sty2900⟩
Monthly Notices of the Royal Astronomical Society, 2019, 483, pp.1808-1828. ⟨10.1093/mnras/sty2900⟩
Quasar accretion-disk outflows might play an important role in galaxy evolution, but they are notoriously difficult to study due to line saturation and blending problems in the Ly-alpha forest. We circumvent these problems by constructing median comp
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::be35147d741ee0eb821de6a69e904a40
Publikováno v:
Frontiers in Astronomy and Space Sciences, Vol 4 (2018)
Accurately determining the masses of supermassive black holes is crucial to understand their evolution and the establishment of their relationship with their host galaxy properties. Beyond the local universe, the single epoch mass estimation method p
Autor:
S. C. Gallagher, Joseph C. Shields, Daniel M. Capellupo, S. M. McGraw, Fred Hamann, W. N. Brandt
Publikováno v:
Physics and Astronomy Publications
FeLoBALs are a rare class of quasar outflows with low-ionization broad absorption lines (BALs), large column densities, and potentially large kinetic energies that might be important for `feedback' to galaxy evolution. In order to probe the physical
Publikováno v:
IAU Symposium, 9 (S304)
IAU Symposium, 9 (S304)
ISSN:0074-1809
ISSN:1743-9213
ISSN:0074-1809
ISSN:1743-9213
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::2efefb0806a8b9b75f231243d106031b
http://doc.rero.ch/record/299972/files/S1743921314004013.pdf
http://doc.rero.ch/record/299972/files/S1743921314004013.pdf
Autor:
Geoffrey C. Bower, Nathalie Degenaar, Daryl Haggard, Daniel M. Capellupo, Heino Falcke, Sera Markoff, Nanda Rea, Nicolas Choux, Frederick K. Baganoff, Craig O. Heinke, Jason Dexter, P. Chris Fragile, Bill Cotton, Farhad Yusef-Zadeh, Casey J. Law, Gabriele Ponti, J. Neilsen
Publikováno v:
The Astrophysical Journal, 845, 1-13
Astrophysical Journal, 845(1):35. IOP Publishing Ltd.
The Astrophysical Journal, 845, 1, pp. 1-13
Astrophysical Journal, 845(1):35. IOP Publishing Ltd.
The Astrophysical Journal, 845, 1, pp. 1-13
Monitoring of Sagittarius A* from X-ray to radio wavelengths has revealed structured variability --- including X-ray flares --- but it is challenging to establish correlations between them. Most studies have focused on variability in the X-ray and in
Publikováno v:
Astrophys.J.
Astrophys.J., 2017, 836 (1), pp.L8. ⟨10.3847/2041-8213/aa5cac⟩
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2017, 836 (1), pp.L8. ⟨10.3847/2041-8213/aa5cac⟩
Astrophys.J., 2017, 836 (1), pp.L8. ⟨10.3847/2041-8213/aa5cac⟩
The Astrophysical journal letters
The Astrophysical journal letters, Bristol : IOP Publishing, 2017, 836 (1), pp.L8. ⟨10.3847/2041-8213/aa5cac⟩
Angular momentum, or spin, is a fundamental property of black holes (BHs), yet it is much more difficult to estimate than mass or accretion rate (for actively accreting systems). In recent years, high-quality X-ray observations have allowed for detai
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::59d5e727f98b3ef5061411c1fa90cd0c
https://hal.archives-ouvertes.fr/hal-01909444
https://hal.archives-ouvertes.fr/hal-01909444
Autor:
Donald G. York, Fred Hamann, Isabelle Pâris, Alina Streblyanska, H. Herbst, Donald P. Schneider, Daniel M. Capellupo, Jian Ge, W. N. Brandt, Patrick Petitjean
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the Royal Astronomical Society, 2017, 469 (1), pp.323-338. ⟨10.1093/mnras/stx870⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 469 (1), pp.323-338. ⟨10.1093/mnras/stx870⟩
Monthly Notices of the Royal Astronomical Society, 2017, 469 (1), pp.323-338. ⟨10.1093/mnras/stx870⟩
Monthly Notices of the Royal Astronomical Society, Oxford University Press (OUP): Policy P-Oxford Open Option A, 2017, 469 (1), pp.323-338. ⟨10.1093/mnras/stx870⟩
Broad absorption lines (BALs) found in a significant fraction of quasar spectra identify high-velocity outflows that might be present in all quasars and could be a major factor in feedback to galaxy evolution. Understanding the nature of these flows
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83210d995e87abb42ec776fa5829569d
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 446:3427-3446
The physics of active super massive black holes (BHs) is governed by their mass (M_BH), spin (a*) and accretion rate ($\dot{M}$). This work is the first in a series of papers with the aim of testing how these parameters determine the observable attri