VHE gamma-ray emission from the new source HESS J1846-029 is spatially coincident with G29.7-0.3 (also known as Kes 75), one of the youngest composite SNRs in the Galaxy, which …

2007年11月26日 · Kes 75 is likely at distance of 5.1 to 7.5 kpc because the highest HI absorption velocity is at 95 km/s and no absorption is associated with a nearby HI emission peak at 102 …

2001年12月3日 · We have observed the young Galactic supernova remnant Kes 75 with the Chandra X-ray Observatory. This object is one of an increasing number of examples of a shell …

Figure 3. SED of PWN Kes 75. Observed data are shown in color, and the best model fit is shown as a black solid line. Dashed and dotted lines show the contribution of the PWN and …

2022年11月16日 · We report the detection of gamma-ray emission from PWN Kes 75 and PSR J1846-0258. Through modeling the spectral energy distribution incorporating the new Fermi …

We model the dynamical and radiative evolution of the Kes 75 system to estimate the birth properties of the neutron star, the energetics of its progenitor, and properties of the PWN. This …

Observed properties of Kes 75. By studying composite supernova remnants (SNRs), remnants which contain a pulsar wind nebula (PWN), it is possible to estimate physical properties of the...

2022年1月12日 · Kes 75 is a Galactic SNR consisting of a PWN and a partial thermal shell. The PWN is powered by a 0.3 s pulsar (PSR J1846-0258) that has a characteristic age of 723 yr, …

2007年12月26日 · Kes 75 is likely at distance of 5.1 to 7.5 kpc because the highest HI absorption velocity is at 95 km/s and no absorption is associated with a nearby HI emission peak at 102 …

We report the detection of gamma-ray emission from pulsar wind nebula (PWN) Kes 75 and PSR J1846−0258. Through modeling the spectral energy distribution incorporating the new Fermi …