The supernova remnant W49B as seen with H.E.S.S. and Fermi-LAT

H.E.S.S. phase-I observations of the plane of the Milky Way

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Table 2

Parameters for the hadronic scenario.

Model	n_H	s	Δs	p_br	B	W_p
	(cm⁻³)			(GeV c⁻¹)	(μG)	(10⁴⁹ erg)
(a1)	100	1.8	1.0	15	100	12
(a2)	100	2.0	0.8	30	100	11
(a3)	100	2.2	0.7	100	90	12
(a4)	1000	1.8	1.0	15	500	1.1
(a5)	1000	2.0	0.8	30	500	1.1
(a6)	1000	2.2	0.7	100	400	1.1

Notes. K_ep is set to 0.01. The total kinetic energies (E_kin) of the radiating particles (W_e,p) are calculated for E_kin > 100 MeV at an assumed distance of 10 kpc.

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