Abstract
The Tycho’s supernova remnant was observed using the SHALON atmospheric Cherenkov telescope at the Tien Shan High-Altitude Observatory. This object has long been considered to be a candidate for sources of cosmic ray hadrons in the Northern Hemisphere. In [1, 2], the Tycho’s properties were described using the nonlinear kinetic model of cosmic ray acceleration in supernovae remnants. The expected γ-ray flux from π 0-decay extends to energies > 30 eV, whereas the γ-ray photon flux generated by inverse Compton scattering is cut off above several TeV. Therefore, the detection of γ-rays at energies of 10–80 TeV by the SHALON telescope is an indication of their hadron origin. From the SHALON telescope data, additional information on such parameters of the Tycho’s supernova remnant as the distance and interstellar medium density was obtained within the theory [1, 2].
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References
E. G. Berezhko, in Proc. 27th International Cosmic Ray Conference, Hamburg, Germany, 2001 (Copernicus Gesellschaft, Hamburg, 2002), p. 226.
H. J. Völk, E. G. Berezhko, L. T. Ksenofontov and G. P. Rowell, Astron. Astrophys. 396, 649 (2000).
V. G. Sinitsina, …, S. I. Nikolsky, V. Yu. Sinitsina, et al., Izv. Russ. Akad. Nauk Ser. Fiz. 63, 610 (1999).
V. G. Sinitsyna, …, S. I. Nikolsky, V. Yu. Sinitsyna, et al., Nucl. Phys. B (Proc. Suppl.) 97, 219 (2001).
V. G. Sinitsina, …, S. I. Nikolsky, V. Yu. Sinitsina, et al., Izv. Russ. Akad. Nauk Ser. Fiz. 69, 422 (2005).
V. G. Sinitsyna, …, S. I. Nikolsky, V. Yu. Sinitsyna, et al., Int. J. Mod. Phys. A., No. 29, 7026 (2005).
V. G. Sinitsyna, …, S. I. Nikolsky, V. Yu. Sinitsyna, et al., in: Toward a Major Atmospheric Cherenkov Detector — VII, Ed. by B. Degrange, G. Fontain (Ecole Polytechnique, Palaiseau, 2005), p. 105.
V. G. Sinitsyna, …, S. I. Nikolsky, V. Yu. Sinitsyna, et al., Nucl. Phys. B (Proc. Suppl.) 151, 112 (2006).
V. G. Sinitsyna, …, S. I. Nikolsky, and V. Yu. Sinitsyna, in Proc. 20th European Cosmic Ray Symposium, Lisbon, Portugal, 2006 (http://www.lip.pt/events/2006/ecrs/) S5–53.
V. G. Sinitsyna, T. P. Arsov, A. A. Malyshko, et al., Nucl. Phys. B (Proc. Suppl.) 175–176, 455 (2008).
V. G. Sinitsyna, F. I. Musin, S. I. Nikolsky, and V. Yu. Sinitsyna, J. Phys. Soc. Japan, 78,Supplement A, 197 (2009).
V. G. Sinitsyna, A. Y. Alaverdyan, R. M. Mirzafatikhov, et al., Nucl. Phys. B (Proc. Suppl.) 196, 433 (2009).
V. G. Sinitsyna and V. Yu. Sinitsyna, in Proc. of XLIVth Rencontres De Moriond, “Very High Energy Phenomena in the Universe”, La Thuile, Aosta Valley, Italy, February 2009, Ed. by Jacques Dumarchez and Jean Tran Thanh Van (THE GIOI Publishers; Hanoi, Vietnam; 2009), p. 77.
T.-P. Li and Y.-Q. Ma, Astrophys. J. 272, 317 (1983).
H. J. Völk, E. G. Berezhko and L. T. Ksenofontov, in Proc. 29th Int. Cosmic Ray Conf., Pune, India, 2005 (Tata Institute of Fundamental Research, Mumbai, 2005), Vol. 3, p. 235.
E. G. Berezhko, L. T. Ksenofontov, and H. J. Völk, Astrophys. Space Sci. 309, 385 (2007).
J. Prahl and C. Prosch (for the HEGRA Collaboration), in Proc. 25th Int. Cosmic Ray Conf., Durban, 1997 (Wesprint, Potchefstroom, South Africa, 1997), Vol. 3, p. 217.
J. H. Buckley, C.W. Akerlof, D. A. Carter-Lwis, et al., Astron. Astrophys. 329, 639 (1998).
M. Catanese and T. C. Weekes, Preprint No. 4811 (Harvard-Smithsonian Center for Astrophysics, 1999).
H. J. Völk, E. G. Berezhko, and L. T. Ksenofontov, Astron. Astrophys. 483, 529 (2008).
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Original Russian Text © V.G. Sinitsina, S.I. Nikolsky, V.Yu. Sinitsina, G.F. Platonov, 2011, published in Kratkie Soobshcheniya po Fizike, 2011, Vol. 38, No. 4, pp. 3–10.
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Sinitsina, V.G., Nikolsky, S.I., Sinitsina, V.Y. et al. Tycho’s supernova remnant as a source of cosmic rays in our galaxy. Bull. Lebedev Phys. Inst. 38, 91–95 (2011). https://doi.org/10.3103/S1068335611040014
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DOI: https://doi.org/10.3103/S1068335611040014