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https://hdl.handle.net/2440/12434
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DC Field | Value | Language |
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dc.contributor.author | Lin, Y. C. | en |
dc.contributor.author | Bertsch, D. L. | en |
dc.contributor.author | Bloom, S. D. | en |
dc.contributor.author | Esposito, J. A. | en |
dc.contributor.author | Hartman, R. C. | en |
dc.contributor.author | Hunter, S. D. | en |
dc.contributor.author | Kanbach, G. | en |
dc.contributor.author | Kniffen, D. A. | en |
dc.contributor.author | Mayer-Hasselwander, H. A. | en |
dc.contributor.author | Michelson, P. F. | en |
dc.contributor.author | Mukherjee, R. | en |
dc.contributor.author | Muecke, A. | en |
dc.contributor.author | Nolan, P. L. | en |
dc.contributor.author | Pohl, M. | en |
dc.contributor.author | Reimer, Olaf | en |
dc.contributor.author | Schneid, E. J. | en |
dc.contributor.author | Thompson, D. J. | en |
dc.contributor.author | Tompkins, W. F. | en |
dc.date.issued | 1999 | en |
dc.identifier.citation | Astrophysical Journal, 1999; 525(1):191-194 | en |
dc.identifier.issn | 0004-637X | en |
dc.identifier.uri | http://hdl.handle.net/2440/12434 | - |
dc.description.abstract | In current theoretical models of the blazar subclass of active galaxies, the broadband emission consists of two components: a low-frequency synchrotron component with a peak in the IR to X-ray band, and a high-frequency inverse Compton component with a peak in the gamma-ray band. In such models, the gamma-ray spectral index should be correlated with the location of the low-energy peak, with flatter gamma-ray spectra expected for blazars with synchrotron peaks at higher photon energies and vice versa. Using the EGRET-detected blazars as a sample, we examine this correlation and possible uncertainties in its construction. | en |
dc.language.iso | en | en |
dc.rights | © 1999. The American Astronomical Society | en |
dc.subject | gamma rays: general; galaxies: active | en |
dc.title | Egret spectral index and the low-energy peak position in the spectral energy distribution of egret-detected blazars | en |
dc.type | Journal article | en |
dc.identifier.doi | 10.1086/307897 | en |
Appears in Collections: | Physics publications |
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