Zobrazeno 1 - 10
of 20
pro vyhledávání: '"Martin A. Bourne"'
Autor:
Martin A. Bourne, Hsiang-Yi Karen Yang
Publikováno v:
Galaxies, Vol 11, Iss 3, p 73 (2023)
Radio jets and the lobes they inflate are common in cool-core clusters and are known to play a critical role in regulating the heating and cooling of the intracluster medium (ICM). This is an inherently multi-scale problem, and much effort has been m
Externí odkaz:
https://doaj.org/article/01623952752a40c48bb2bcc2ff3da110
Recent observations of Seyfert galaxies indicate that low power, misaligned jets can undergo significant interaction with the gas in the galactic disc and may be able to drive large-scale, multiphase outflows. We apply our novel sub-grid model for Bl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1c8c4dbe0fe28c912c4330d1cd3f574a
http://arxiv.org/abs/2111.01801
http://arxiv.org/abs/2111.01801
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Jets launched by active galactic nuclei (AGN) are believed to play a significant role in shaping the properties of galaxies and provide an energetically viable mechanism through which galaxies can become quenched. Here we present a novel AGN feedback
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::011dc4762664caf063a7415932759cc3
https://www.repository.cam.ac.uk/handle/1810/350946
https://www.repository.cam.ac.uk/handle/1810/350946
Autor:
Debora Sijacki, Martin A. Bourne
Publikováno v:
Monthly Notices of the Royal Astronomical Society
While there is overwhelming observational evidence of AGN-driven jets in galaxy clusters and groups, if and how the jet energy is delivered to the ambient medium remains unanswered. Here we perform very high resolution AGN jet simulations within a li
Autor:
Martin Albert Bourne
Publikováno v:
Proceedings of the International Astronomical Union. 12:231-234
Feedback released during the growth of supermassive black holes is expected to play a key role in shaping black hole-host galaxy co-evolution. Powerful, accretion disc driven winds have been invoked to explain both observed scaling relations (e.g., M
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Jet feedback from active galactic nuclei (AGN) harboured by brightest cluster galaxies is expected to play a fundamental role in regulating cooling in the intracluster medium (ICM). While observations and theory suggest energy within jet lobes balanc
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::11da70a30b6911265db40c3252ab66a4
http://arxiv.org/abs/1901.11030
http://arxiv.org/abs/1901.11030
Autor:
Giacomo Venturi, Alessandro Marconi, A. Fluetsch, W. Ishibashi, Andrew C. Fabian, Claudia Cicone, Roberto Maiolino, Stefano Carniani, Tiago Costa, Martin A. Bourne
Publikováno v:
Monthly Notices of the Royal Astronomical Society
Monthly Notices of the RAS (0035-8711), 483(4), 4586-4614
Monthly Notices of the RAS (0035-8711)
Monthly Notices of the RAS (0035-8711), 483(4), 4586-4614
Monthly Notices of the RAS (0035-8711)
We study molecular outflows in a sample of 45 local galaxies, both star forming and active galactic nucleus (AGN), primarily by using CO data from the Atacama Large Millimeter/submillimeter Array (ALMA) archive and from the literature. For a subsampl
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1d1979595e7bfd644523312779993407
https://www.repository.cam.ac.uk/handle/1810/289275
https://www.repository.cam.ac.uk/handle/1810/289275
Publikováno v:
Monthly Notices of the Royal Astronomical Society
The systematic analysis of optical large-scale surveys has revealed a population of dwarf galaxies hosting AGN, which have been confirmed by X-ray follow-up observations. Recently, the MaNGA survey identified six dwarf galaxies that appear to have an
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 453:1829-1842
Feedback from super-massive black holes (SMBHs) is thought to play a key role in regulating the growth of host galaxies. Cosmological and galaxy formation simulations using smoothed particle hydrodynamics (SPH), which usually use a fixed mass for SPH
Autor:
Kastytis Zubovas, Martin A. Bourne
Publikováno v:
Monthly Notices of the Royal Astronomical Society
AGN outflows can remove large quantities of gas from their host galaxy spheroids, potentially shutting off star formation. On the other hand, they can compress this gas, potentially enhancing or triggering star formation, at least for short periods.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::f63fc76edbbed408a64241ba2ca066e6
http://arxiv.org/abs/1703.10782
http://arxiv.org/abs/1703.10782