Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Jo-Anne C. Brown"'
Autor:
Nasser Mohammed, Anna Ordog, Rebecca A. Booth, Andrea Bracco, Jo-Anne C. Brown, Ettore Carretti, John M. Dickey, Simon Foreman, Mark Halpern, Marijke Haverkorn, Alex S. Hill, Gary Hinshaw, Joseph W. Kania, Roland Kothes, T. L. Landecker, Joshua MacEachern, Kiyoshi W. Masui, Aimee Menard, Ryan R. Ransom, Wolfgang Reich, Patricia Reich, J. Richard Shaw, Seth R. Siegel, Mehrnoosh Tahani, Alec J. M. Thomson, Tristan Pinsonneault-Marotte, Haochen Wang, Jennifer L. West, Maik Wolleben, Dallas Wulf, CHIME and GMIMS Collaborations
Publikováno v:
The Astrophysical Journal, Vol 971, Iss 1, p 100 (2024)
A direct consequence of Faraday rotation is that the polarized radio sky does not resemble the total intensity sky at long wavelengths. We analyze G137+7, which is undetectable in total intensity but appears as a depolarization feature. We use the fi
Externí odkaz:
https://doaj.org/article/a391268e73a74d42872dff194de6cf75
Publikováno v:
Galaxies, Vol 7, Iss 2, p 43 (2019)
The Galactic magnetic field is an integral constituent of the interstellar medium (ISM), and knowledge of its structure is crucial to understanding Galactic dynamics. The Rotation Measures (RM) of extragalactic (EG) sources have been the basis of com
Externí odkaz:
https://doaj.org/article/f3451e956af84efdad13805d4cacb0a4
Autor:
John M. Dickey, Jennifer West, Alec J. M. Thomson, T. L. Landecker, A. Bracco, E. Carretti, J. L. Han, A. S. Hill, Y. K. Ma, S. A. Mao, A. Ordog, Jo-Anne C. Brown, K. A. Douglas, A. Erceg, V. Jelić, R. Kothes, M. Wolleben
Magnetic fields in the ionized medium of the disk and halo of the Milky Way impose Faraday rotation on linearly polarized radio emission. We compare two surveys mapping the Galactic Faraday rotation, one showing the rotation measures of extragalactic
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::38ec2809bd2e4e02028816edce3b5046
http://arxiv.org/abs/2209.10819
http://arxiv.org/abs/2209.10819
Autor:
Aurélien A. Fraisse, Jo-Anne C. Brown, Gregory Dobler, Jessie L. Dotson, Bruce T. Draine, Priscilla C. Frisch, Marijke Haverkorn, Christopher M. Hirata, Ronnie Jansson, Alex Lazarian, Antonio Mario Magalhães, André Waelkens, Maik Wolleben, Scott Dodelson, Chryssa Baumann, Asantha Cooray, Joanna Dunkley, Aurelien Fraisse, Mark G. Jackson, Alan Kogut, Lawrence Krauss, Matias Zaldarriaga, Kendrick Smith
Publikováno v:
ResearcherID
Detecting “B‐mode” (i.e., divergence free) polarization in the Cosmic Microwave Background (CMB) would open a new window on the very early Universe. However, the polarized microwave sky is dominated by polarized Galactic dust and synchrotron em
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::66da5e51bc1f8c7ed5a0e531f28b6f5d
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=ORCID&SrcApp=OrcidOrg&DestLinkType=FullRecord&DestApp=WOS_CPL&KeyUT=WOS:000270939500006&KeyUID=WOS:000270939500006
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcAuth=ORCID&SrcApp=OrcidOrg&DestLinkType=FullRecord&DestApp=WOS_CPL&KeyUT=WOS:000270939500006&KeyUID=WOS:000270939500006