Craig L. Sarazin
University of Virginia
474 Papers
5.1K Citations
Craig L. Sarazin is an academic researcher from University of Virginia. The author has contributed to research in topics: Galaxy & Galaxy cluster. The author has an hindex of 72, co-authored 449 publications. Previous affiliations of Craig L. Sarazin include National Institute of Standards and Technology & National Radio Astronomy Observatory.
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Papers
Geometry of the Draco C1 Symbiotic Binary
Hannah M. Lewis,Borja Anguiano,Keivan G. Stassun,Steven R. Majewski,Phil Arras,Craig L. Sarazin,Zhi-Yun Li,Nathan De Lee,Nathan De Lee,Nicholas W. Troup,Carlos Allende Prieto,Carlos Allende Prieto,Carles Badenes,Katia Cunha,D. A. García-Hernández,D. A. García-Hernández,David L. Nidever,Pedro A. Palicio,Pedro A. Palicio,Pedro A. Palicio,Joshua D. Simon,Verne V. Smith +21 more
TL;DR: In this article, the authors derived the orbital period of a known symbiotic binary star system composed of a carbon red giant and a hot, compact companion, belonging to the Draco dwarf spheroidal galaxy.
A merger shock in Abell 1367
Chong Ge,Ming Sun,Ruo Yu Liu,Lawrence Rudnick,Craig L. Sarazin,William R. Forman,Christine Jones,Hao Chen,Wenhao Liu,Masafumi Yagi,Alessandro Boselli,Matteo Fossati,Giuseppe Gavazzi +12 more
TL;DR: In this paper, a previously unknown merger shock at the NW edge of Abell 1367 (A1367) was discovered, which could be produced by the re-acceleration of pre-existing seed relativistic electrons.
X-Ray Evidence for the Interaction of the Giant Elliptical Galaxy NGC 4472 with its Virgo Cluster Environment
Jimmy A. Irwin,Craig L. Sarazin +1 more
TL;DR: In this article, the authors analyzed X-ray spatial and spectral data on the giant elliptical galaxy NGC 4472, the brightest galaxy in the Virgo cluster, and found that the majority of the material in the cloud is molecular.
Chandra Observations of the Disruption of the Cool Core in A133
Yutaka Fujita,Craig L. Sarazin,Joshua C. Kempner,Lawrence Rudnick,O. B. Slee,Alan L. Roy,Heinz Andernach,Matthias Ehle +7 more
TL;DR: In this paper, the authors present the analysis of a Chandra observation of the galaxy cluster A133, which has a cooling flow core, a central radio source and a diffuse, filamentary radio source that has been classified as a radio relic.
Abundance gradients in extragalactic H II regions and internal absorption by dust
TL;DR: In this article, the radio, optical, and infrared observations of giant spiral arm H II regions in the Sc galaxies M33, M51, and M101 are discussed, in order to determine the effect of the observed abundance gradients on the structure of the regions.