Kenneth W. Cavagnolo, Ph.D.
Affiliations: | 2008 | Michigan State University, East Lansing, MI |
Area:
Astronomy and AstrophysicsGoogle:
"Kenneth Cavagnolo"Mean distance: (not calculated yet)
Parents
Sign in to add mentor| Megan Elizabeth Donahue | grad student | 2008 | Michigan State | |
| (Investigating feedback and relaxation in clusters of galaxies with the Chandra X -ray Observatory.) | ||||
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Publications
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| Cavagnolo KW, Donahue M, Voit GM, et al. (2009) Intracluster medium entropy profiles for a chandra archival sample of galaxy clusters Astrophysical Journal, Supplement Series. 182: 12-32 |
| Cavagnolo KW, Donahue M, Voit GM, et al. (2008) An entropy threshold for strong ha and radio emission in the cores of galaxy clusters Astrophysical Journal. 683 |
| Voit GM, Cavagnolo KW, Donahue M, et al. (2008) Conduction and the star formation threshold in brightest cluster galaxies Astrophysical Journal. 681 |
| Cavagnolo KW, Donahue M, Voit GM, et al. (2008) Bandpass Dependence of X-Ray Temperatures in Galaxy Clusters The Astrophysical Journal. 682: 821-834 |
| Donahue M, Ming S, O'Dea CP, et al. (2007) Star formation, radio sources, cooling x-ray gas, and galaxy interactions in the brightest cluster galaxy in 2A0335+096 Astronomical Journal. 134: 14-25 |
| Sharpee B, Zhang Y, Williams R, et al. (2007) s-PROCESS ABUNDANCES IN PLANETARY NEBULAE The Astrophysical Journal. 659: 1265-1290 |
| Donahue M, Horner DJ, Cavagnolo KW, et al. (2006) Entropy profiles in the cores of cooling flow clusters of galaxies Astrophysical Journal. 643: 730-750 |
| Zhang Y, Williams R, Pellegrini E, et al. (2006) Abundances of s-process elements in planetary nebulae: Br, Kr & Xe Arxiv: Astrophysics. 2: 549-550 |