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
Rapid compact jet quenching in the Galactic black hole candidate X-ray binary MAXI J1535-571
Thomas D. Russell,Marco Toliman Lucchini,Alexandra J. Tetarenko,James Miller-Jones,G. R. Sivakoff,Felicia Krauß,Felicia Krauß,Wanga Mulaudzi,Maria Cristina Baglio,Maria Cristina Baglio,D. M. Russell,Diego Altamirano,Chiara Ceccobello,Stephane Corbel,Stephane Corbel,Nathalie Degenaar,J. van den Eijnden,Rob Fender,Sebastian Heinz,Karri I. I. Koljonen,Karri I. I. Koljonen,D. Maitra,Sera Markoff,Simone Migliari,Aastha S. Parikh,Richard M. Plotkin,Michael P. Rupen,Craig L. Sarazin,Roberto Soria,Roberto Soria,Rudy Wijnands +30 more
TL;DR: In this paper, the authors present results from six epochs of quasi-simultaneous radio, (sub-) millimetre, infrared, optical, and X-ray observations of the black hole Xray binary MAXI J1535-571.
Dynamics of Kepler's supernova remnant
TL;DR: In this article, the authors studied the dynamics of supernova ejecta interaction with the dense circumstellar medium (CSM) and identified the transmitted shock with the nonradiative, Balmerdominated shocks found recently in Kepler's SNR.
Untangling the X-Ray Emission from the Sa Galaxy NGC 1291 with Chandra
TL;DR: In this paper, Chandra ACIS-S observations of the nearby bulge-dominated Sa galaxy NGC 1291 were used to detect low-mass X-ray binaries (LMXBs) and diffuse gas detectable out to a radius of 120'' (5.2 kpc).
An Alignment Effect in FR I Radio Galaxies: U-Band Polarimetry of the Abell 2597 Cluster Central Galaxy
Brian R. McNamara,Brian R. McNamara,Buell T. Jannuzi,Craig L. Sarazin,Richard Elston,Michael W. Wise +5 more
TL;DR: In this article, U-band polarimetry of the spatially extended blue optical continuum associated with the FR I radio source PKS 2322-122, located in the Abell 2597 cluster central galaxy, was obtained.
Chandra Observation of Abell 2065: An Unequal Mass Merger?
TL;DR: In this article, the authors present an analysis of a 41 ks Chandra ACIS-I observation of the merging cluster Abell 2065 and argue that only one of the two cooling cores has survived the merger, placing an upper limit of 1900 km s-1 on the relative merger velocity.