Distances to Two Galactic Supernova Remnants: G32.8-0.1 and G346.6-0.2

Details Distances to Two Galactic Supernova Remnants: G32.8-0.1 and G346.6-0.2 Distances to Two Galactic Supernova Remnants: G32.8-0.1 and G346.6-0.2

2009-09-02

arxiv.org/abs/0909.0394v1

Astronomy and Astrophysics

Astrophysics

High Energy Astrophysical Phenomena

5 pages, 3 figures

Scientific paper

There are either a near kinematic distance of 5.5 kpc or a far distance of 8.8 kpc for a Galactic supernova remnant (SNR) G32.8$-$0.1 derived by using the rotation curve of the Galaxy. Here we make sure that the remnant distance is the farther one 8.8 kpc through solving a group of equations for the shell-type remnants separately at the adiabatic-phase and the radiative-phase. For SNR G346.6$-$0.2 we determine its distance also the farther one 11 kpc rather than the nearer one 5.5 kpc.

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