TWELVE AND A HALF YEARS OF OBSERVATIONS OF CENTAURUS A WITH THE ROSSI X-RAY TIMING EXPLORER
dc.contributor.author | Rothschild, R. E. | |
dc.contributor.author | Markowitz, A. | |
dc.contributor.author | Rivers, E. | |
dc.contributor.author | Suchy, S. | |
dc.contributor.author | Pottschmidt, Katja | |
dc.contributor.author | Kadler, M. | |
dc.contributor.author | Müller, C. | |
dc.contributor.author | Wilms, J. | |
dc.date.accessioned | 2023-09-22T16:09:44Z | |
dc.date.available | 2023-09-22T16:09:44Z | |
dc.date.issued | 2011-04-29 | |
dc.description.abstract | The Rossi X-ray Timing Explorer (RXTE) has observed the nearest radio galaxy, Centaurus A (Cen A), in 13 intervals from 1996 August to 2009 February over the 3–200 keV band. Spectra accumulated over the 13 intervals were well described with an absorbed power law and an iron line. Cutoff power laws and Compton reflection from cold matter did not provide a better description. For the 2009 January observation, we set a lower limit on the cutoff energy at over 2 MeV. The power spectral density function was generated from RXTE/All Sky Monitor and Proportional Counter Array data as well as an XMM-Newton long look, and clear evidence for a break at 18⁺¹⁸₋₇ days (68% conf.) was seen. Given Cen A's high black hole mass and very low value of LX/LEdd, the break was a factor of 17⁺³⁶₋₁₃ times higher than the break frequency predicted by the McHardy et al. relation, which was empirically derived for a sample of objects, which are radio-quiet and accreting at relatively high values of Lbol/LEdd. We have interpreted our observations in the context of a clumpy molecular torus. The variability characteristics and the broadband spectral energy distribution, when compared to Seyferts, imply that the bright hard X-ray continuum emission may originate at the base of the jet, yet from behind the absorbing line-of-sight material, in contrast to what is commonly observed from blazars. | en_US |
dc.description.sponsorship | The authors acknowledge the excellent comments from the anonymous referee. We gratefully acknowledge NASA contract NAG5-30720 and NASA grants NNX08AY11G and NNX09AG79G for support of this analysis. | en_US |
dc.description.uri | https://iopscience.iop.org/article/10.1088/0004-637X/733/1/23 | en_US |
dc.format.extent | 19 pages | en_US |
dc.genre | journal articles | en_US |
dc.identifier | doi:10.13016/m2kigx-chf5 | |
dc.identifier.citation | Rothschild, R. E., A. Markowitz, E. Rivers, S. Suchy, K. Pottschmidt, M. Kadler, C. Müller, and J. Wilms. “TWELVE AND A HALF YEARS OF OBSERVATIONS OF CENTAURUS A WITH THE ROSSI X-RAY TIMING EXPLORER.” The Astrophysical Journal 733, no. 1 (April 2011): 23. https://doi.org/10.1088/0004-637X/733/1/23. | en_US |
dc.identifier.uri | https://doi.org/10.1088/0004-637X/733/1/23 | |
dc.identifier.uri | http://hdl.handle.net/11603/29836 | |
dc.language.iso | en_US | en_US |
dc.publisher | IOP Publishing | en_US |
dc.relation.isAvailableAt | The University of Maryland, Baltimore County (UMBC) | |
dc.relation.ispartof | UMBC Center for Space Sciences and Technology | |
dc.relation.ispartof | UMBC Faculty Collection | |
dc.relation.ispartof | UMBC Physics Department | |
dc.rights | This item is likely protected under Title 17 of the U.S. Copyright Law. Unless on a Creative Commons license, for uses protected by Copyright Law, contact the copyright holder or the author. | en_US |
dc.title | TWELVE AND A HALF YEARS OF OBSERVATIONS OF CENTAURUS A WITH THE ROSSI X-RAY TIMING EXPLORER | en_US |
dc.type | Text | en_US |
dcterms.creator | https://orcid.org/0000-0002-4656-6881 | en_US |