Zobrazeno 1 - 10
of 21
pro vyhledávání: '"E. M. Douglass"'
Autor:
Courtney B. Watson, Elizabeth L. Blanton, Scott W. Randall, Craig L. Sarazin, Arnab Sarkar, John A. ZuHone, E. M. Douglass
Publikováno v:
The Astrophysical Journal, Vol 955, Iss 2, p 103 (2023)
We present Chandra X-ray observations of the dynamically complex galaxy cluster A119 ( z = 0.044). A119 is host to two narrow-angle-tail (NAT) radio sources (0053-015 and 0053-016), whose tails are oriented parallel to each other, despite orthogonall
Externí odkaz:
https://doaj.org/article/8fd28541c2c546768b3be8b5940d57a2
Autor:
Scott W. Randall, Tracy Clarke, Elizabeth L. Blanton, Louise O. V. Edwards, Z. Sabry, John ZuHone, E. M. Douglass
We present a multiwavelength study of the massive galaxy cluster Abell 1763 at redshift z = 0.231. Image analysis of a 19.6 ks Chandra archival observation reveals a cluster-wide spiral of enhanced surface brightness in the intracluster medium (ICM).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::05cab16bd0a952d60fc692adcd06b074
Autor:
James G. Richman, E. M. Douglass
Publikováno v:
Journal of Geophysical Research: Oceans. 120:1490-1507
Strongly nonlinear surface eddies are identified and analyzed in a general circulation model. Agulhas rings and Gulf Stream cold-core eddies are examples of eddies that cannot be properly characterized using linear geostrophic dynamics. These eddies
Autor:
Emmet Golden-Marx, Mark Brodwin, Tracy Clarke, Joshua D. Wing, Scott W. Randall, E. M. Douglass, M. L. N. Ashby, Rachel Paterno-Mahler, Elizabeth L. Blanton
Publikováno v:
Proceedings of the International Astronomical Union. 10:315-320
We are conducting a large survey of distant clusters of galaxies using radio sources with bent jets and lobes as tracers. These radio sources are driven by AGN and achieve their bent morphologies through interaction with the surrounding gas found in
Autor:
Craig L. Sarazin, Elizabeth L. Blanton, E. M. Douglass, Tracy E. Clarke, Gopal-Krishna, Namir E. Kassim, L. D. Anderson
Publikováno v:
The Astrophysical Journal. 697:1481-1492
We present new radio and X-ray observations of Abell 262. The X-ray residual image provides the first evidence of an X-ray tunnel in this system while the radio data reveal that the central radio source is more than three times larger than previously
Publikováno v:
Astrophysical Journal, 673(2), 763-777. IOP Publishing Ltd.
Wide-angle tail (WAT) radio sources are often found in the centers of galaxy clusters where intracluster medium (ICM) ram pressure may bend the lobes into their characteristic C-shape. We examine the low redshift (z=0.1035) cluster Abell 1446, host t
Autor:
Craig L. Sarazin, Scott W. Randall, Tracy E. Clarke, E. M. Douglass, Michael McDonald, Elizabeth L. Blanton, Brian R. McNamara
We present first results from a very deep (~650 ksec) Chandra X-ray observation of Abell 2052, as well as archival VLA radio observations. The data reveal detailed structure in the inner parts of the cluster, including bubbles evacuated by the AGN's
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6c019f057589306575eb12e27e94a12f
http://arxiv.org/abs/1105.4572
http://arxiv.org/abs/1105.4572
Autor:
Brian R. McNamara, Elizabeth L. Blanton, Craig L. Sarazin, Scott W. Randall, Tracy Clarke, E. M. Douglass
We present results from a deep Chandra observation of Abell 2052. A2052 is a bright, nearby, cooling flow cluster, at a redshift of z=0.035. Concentric surface brightness discontinuities are revealed in the cluster center, and these features are cons
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7ba7d03d4c623e7ec01995fdfdc404db
Publikováno v:
Eso Astrophysics Symposia ISBN: 9783540734833
We present initial results from a long (125 ksec) Chandra observation of Abell 2052. A2052 is a bright, nearby, cooling core cluster at a redshift of z=0.0348. It was previously observed for 36 ksec with Chandra [3,4]. The longer observation reveals
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b0c5d086058df16e9e1fe8add8d8674f
https://doi.org/10.1007/978-3-540-73484-0_20
https://doi.org/10.1007/978-3-540-73484-0_20
Publikováno v:
The Astrophysical Journal. 743:199
We present a Chandra X-ray observation and Very Large Array radio observations of the nearby (z = 0.11) galaxy cluster A562 and the wide angle tail (WAT) radio source 0647+693. The cluster displays signatures of an ongoing merger leading to the bendi