An energy-conserving, particle-dominated, time-dependent model of 3C 58 and its observability at high energies
We present a time-dependent spectral model of the nebula 3C 58 and compare it with available data. The model is for a leptonic nebula in which particles are subject to synchrotron, inverse Compton, self-synchrotron Compton, adiabatic, and bremsstrahlung processes. We find that 3C 58 is compatible wi...
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| Formato: | Capítulo de libro |
| Lenguaje: | Inglés |
| Publicado: |
The American Astronomical Society
2013
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| Acceso en línea: | Registro en Scopus DOI Handle Registro en la Biblioteca Digital |
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| LEADER | 08405caa a22008777a 4500 | ||
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| 001 | PAPER-27063 | ||
| 003 | AR-BaUEN | ||
| 005 | 20230711124140.0 | ||
| 008 | 190410s2013 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-84872282817 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Torres, D.F. |4 aut |e autor | |
| 245 | 1 | 3 | |a An energy-conserving, particle-dominated, time-dependent model of 3C 58 and its observability at high energies |
| 260 | |c 2013 |b The American Astronomical Society | ||
| 270 | 1 | 0 | |m Torres, D.F.; Institute of Space Sciences (IEEC-CSIC), Campus UAB, Torre C5, 2a planta, E-08193 Barcelona, Spain |
| 506 | |2 openaire |e Política editorial |f info:eu-repo/semantics/openAccess | ||
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| 520 | 3 | |a We present a time-dependent spectral model of the nebula 3C 58 and compare it with available data. The model is for a leptonic nebula in which particles are subject to synchrotron, inverse Compton, self-synchrotron Compton, adiabatic, and bremsstrahlung processes. We find that 3C 58 is compatible with being a particle-dominated nebula, with a magnetic field of 35 μG. A broken power-law injection fits well the multi-frequency data, with a break energy at about 40 GeV. We find that 3C 58 is not expected to appear in VERITAS or MAGIC II, unless the local IR background is a factor of ∼20 off Galactic models' averages. For cases in which the cosmic microwave background dominates the inverse Compton contribution, we find that 3C 58 will not be visible either for the Cherenkov Telescope Array. © 2013. The American Astronomical Society. All rights reserved. |l eng | |
| 593 | |a Institute of Space Sciences (IEEC-CSIC), Campus UAB, Torre C5, 2a planta, E-08193 Barcelona, Spain | ||
| 593 | |a Institució Catalana de Recerca i Estudis Avançats (ICREA), E-08010 Barcelona, Spain | ||
| 593 | |a Instituto de Astronomía y Física Del Espacio, Casilla de Correo 67-Suc. 28 (C1428ZAA), Buenos Aires, Argentina | ||
| 690 | 1 | 0 | |a ISM: INDIVIDUAL OBJECTS: (3C 58) |
| 700 | 1 | |a Cillis, A.N. |4 aut |e autor | |
| 700 | 1 | |a Martín Rodriguez, J. |4 aut |e autor | |
| 773 | 0 | |d 2013 |g v. 763 |k n. 1 |p Astrophys. J. Lett. |x 20418205 |t Astrophysical Journal Letters | |
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