Zobrazeno 1 - 10
of 21
pro vyhledávání: '"Sui Ann Mao"'
Autor:
Enrique Lopez-Rodriguez, Alejandro S. Borlaff, Rainer Beck, William T. Reach, Sui Ann Mao, Evangelia Ntormousi, Konstantinos Tassis, Sergio Martin-Alvarez, Susan E. Clark, Daniel A. Dale, Ignacio del Moral-Castro
Publikováno v:
The Astrophysical Journal Letters, Vol 942, Iss 1, p L13 (2022)
Mergers are thought to be a fundamental channel for galaxy growth, perturbing the gas dynamics and the magnetic fields ( B -fields) in the interstellar medium (ISM). However, the mechanisms that amplify and dissipate B -fields during a merger remain
Externí odkaz:
https://doaj.org/article/67a3f81e056749f687b0238605a0b75e
Autor:
George Heald, Sui Ann Mao, Valentina Vacca, Takuya Akahori, Ancor Damas-Segovia, B. M. Gaensler, Matthias Hoeft, Ivan Agudo, Aritra Basu, Rainer Beck, Mark Birkinshaw, Annalisa Bonafede, Tyler L. Bourke, Andrea Bracco, Ettore Carretti, Luigina Feretti, J. M. Girart, Federica Govoni, James A. Green, JinLin Han, Marijke Haverkorn, Cathy Horellou, Melanie Johnston-Hollitt, Roland Kothes, Tom Landecker, Błażej Nikiel-Wroczyński, Shane P. O’Sullivan, Marco Padovani, Frédérick Poidevin, Luke Pratley, Marco Regis, Christopher John Riseley, Tim Robishaw, Lawrence Rudnick, Charlotte Sobey, Jeroen M. Stil, Xiaohui Sun, Sharanya Sur, A. Russ Taylor, Alec Thomson, Cameron L. Van Eck, Franco Vazza, Jennifer L. West, the SKA Magnetism Science Working Group
Publikováno v:
Galaxies, Vol 8, Iss 3, p 53 (2020)
The Square Kilometre Array (SKA) will answer fundamental questions about the origin, evolution, properties, and influence of magnetic fields throughout the Universe. Magnetic fields can illuminate and influence phenomena as diverse as star formation,
Externí odkaz:
https://doaj.org/article/9fbcce7800434bca9f1ed1306b7a9475
Publikováno v:
Galaxies, Vol 5, Iss 4, p 66 (2017)
As radio polarised emission from astrophysical objects traverse through foreground magnetised plasma, the physical conditions along the lines of sight are encrypted in the form of rotation measure (RM). We performed broadband spectro-polarimetric obs
Externí odkaz:
https://doaj.org/article/336fccd958ae40829b82d4abd92cfad5
Autor:
Steve Croft, Tessa Vernstrom, Charles L. H. Hull, M. C. H. Wright, A. Clegg, Peter Williams, Bryan Gaensler, Jane F. Kaczmarek, George Heald, Subhashis Roy, Timothy W. Shimwell, C. Tasse, Allison H. Costa, G. C. Bower, Yik Ki Ma, C. J. Riseley, Makoto Inoue, Shane O'Sullivan, Torsten A. Enßlin, Charlotte Sobey, Sui Ann Mao, Jeroen Stil, Marcus Brüggen, C. J. Law, M. Haverkorn, Tracy E. Clarke, F. de Gasperin, C. L. Van Eck, R. Shanahan, Craig S. Anderson, V. Vacca, S. K. Betti, Sebastian Hutschenreuter, Jo-Anne Brown, Melanie Johnston-Hollitt, E. Carretti, Dave MacMahon
Publikováno v:
Astronomy & Astrophysics, 657, 1-14
Astronomy & Astrophysics, 657:A43
Astronomy & Astrophysics, 657, pp. 1-14
Astronomy & Astrophysics, 657:A43
Astronomy & Astrophysics, 657, pp. 1-14
This work gives an update to existing reconstructions of the Galactic Faraday rotation sky by processing almost all Faraday rotation data sets available at the end of the year 2020. Observations of extra-Galactic sources in recent years have, among o
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb34861166d0495863684e0e2f62f622
http://hdl.handle.net/2066/246381
http://hdl.handle.net/2066/246381
Autor:
Dominic Schnitzeler, Blakesley Burkhart, Sui Ann Mao, Rainer Beck, Andrew Fletcher, Aritra Basu
Publikováno v:
Galaxies
Volume 7
Issue 4
Volume 7
Issue 4
In this paper we present a detailed analysis of the Faraday depth (FD) spectrum and its clean components obtained through the application of the commonly used technique of Faraday rotation measure synthesis to analyze spectro-polarimetric data. In or
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::1453926cd059ca03ad9535b5bcb90871
Publikováno v:
ASP Conference Series; 2020, Vol. 528, p61-66, 6p
Autor:
Andrew Fletcher, Sui Ann Mao
Publikováno v:
Nature Astronomy. 3:965-966
Seventy years after the first detection of interstellar magnetic fields, experts met in Newcastle upon Tyne, UK, on 10–14 June 2019, to discuss new perspectives on interstellar magnetic fields from small to large scales, from the Milky Way to dista
Autor:
M. Haverkorn, G. J. Madsen, Bryan Gaensler, Phil Kronberg, Sui Ann Mao, Ellen G. Zweibel, Naomi McClure-Griffiths, Anvar Shukurov
Publikováno v:
The Astrophysical Journal. 714:1170-1186
We present a study of the vertical magnetic field of the Milky Way towards the Galactic poles, determined from observations of Faraday rotation toward more than 1000 polarized extragalactic radio sources at Galactic latitudes |b| > 77 degs, using the
Autor:
Timothy Robishaw, Sui Ann Mao, Xiaohui Sun, Peter Frick, T. L. Landecker, Marijke Haverkorn, Rodion Stepanov, A. Noutsos, Takuya Akahori, Dominic Schnitzeler, Katia Ferrière, Ettore Carretti, Wolfgang Reich, George Heald, Niels Oppermann, Anna M. M. Scaife, Melanie Johnston-Hollitt, Bryan Gaensler, David J. Jones, Russ Taylor
Publikováno v:
Scopus-Elsevier
Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 9-13 June, 2014. Giardini Naxos, Italy. Online at http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=215, id.96. SKA Organisation
Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 9-13 June, 2014. Giardini Naxos, Italy. Online at http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=215, id.96
STARTPAGE=96;TITLE=None
NASA Astrophysics Data System
Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 9-13 June, 2014. Giardini Naxos, Italy. Online at http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=215, id.96. SKA Organisation
Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 9-13 June, 2014. Giardini Naxos, Italy. Online at http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=215, id.96
STARTPAGE=96;TITLE=None
NASA Astrophysics Data System
Magnetic fields in the Milky Way are present on a wide variety of sizes and strengths, influencing many processes in the Galactic ecosystem such as star formation, gas dynamics, jets, and evolution of supernova remnants or pulsar wind nebulae. Observ
Autor:
Cathy Horellou, Rosita Paladino, Dmitry Sokoloff, Katia Ferrière, Yu-Qing Lou, Sui Ann Mao, George Heald, Dominik J. Bomans, Marita Krause, Eva Schinnerer, Jeroen M. Stil, Ralf-Jürgen Dettmar, Fatemeh Tabatabaei, Rainer Beck, Andrew Fletcher, Sergio Colafrancesco, Volker Heesen
Publikováno v:
Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 9-13 June, 2014. Giardini Naxos, Italy. Online at http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=215, id.94. SKA Organisation
Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 9-13 June, 2014. Giardini Naxos, Italy. Online at http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=215, id.94
NASA Astrophysics Data System
Scopus-Elsevier
Proceedings of Advancing Astrophysics with the Square Kilometre Array (AASKA14). 9-13 June, 2014. Giardini Naxos, Italy. Online at http://pos.sissa.it/cgi-bin/reader/conf.cgi?confid=215, id.94
NASA Astrophysics Data System
Scopus-Elsevier
Magnetic fields are an important ingredient of the interstellar medium (ISM). Besides their importance for star formation, they govern the transport of cosmic rays, relevant to the launch and regulation of galactic outflows and winds, which in turn a
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d6bf38972877d18127171cd622ae8da1
http://arxiv.org/abs/1501.00385
http://arxiv.org/abs/1501.00385