We performed HI 21 cm line observations in a field around the SNR 3C 400.2 with the DRAO Synthesis Telescope.
These observations revealed the existence
of neutral gas features associated with the remnant. Namely:
i) a clumpy HI cloud delineating the north, west and southern border
of 3C 400.2 in the velocity range +14 to +42 km s-1 and ii) gas
probably accelerated by the shock front at v=-49.5 and +69 km s-1.
A simple picture that can explain the observed morphology
of 3C 400.2 in the different spectral regimes is as follows:
the remnant originated from a supernova explosion occurring
near the border of a neutral gas cloud approximately 21 cm-3
in density.
The position of the explosion
coincides with the center of the HI
void detected at v=+27 km s-1 and with the geometrical center of the
bright optical filaments.
The "small NW shell" evolved
within the dense cloud until it broke out originating the "large radio
shell" where it is evolving into a medium about five times lighter.
We argue that the optical filaments originated in regions where
the front shock encountered and overtook density enhancements in the surrounding
interstellar medium. The excellent correspondence between regions of H emission with regions of enhanced HI emission detected between +26 and
+28 km s-1 confirms this scenario. By comparing the HI observations with the
X-ray image, we found a hole in the HI distribution at +28 km s-1 coinciding
exactly with the maximum in the X-ray emission, this suggests that the
neutral gas could have been partially evaporated thus producing centrally
condensed X-ray morphology.
From the present observations a distance of 2.8 0.8 kpc
to 3C 400.2 was calculated.
We would like to thank Dr. Tom Landecker for his valuable contribution in the first stages of this work. E.B.G. thanks DRAO for support and the kind hospitality during her visit to Penticton. The Dominion Radio Astrophysical Observatory Synthesis Telescope is operated as a national facility by the National Research Council of Canada. This research was supported by the CONICET grant PMT-PICT 0107.
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