Far Ultraviolet Observation of the Monogem Ring

Details Far Ultraviolet Observation of the Monogem Ring Far Ultraviolet Observation of the Monogem Ring

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aas...21012304k&link_type=abstract

American Astronomical Society Meeting 210, #123.04; Bulletin of the American Astronomical Society, Vol. 39, p.332

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Scientific paper

We present the results of the far ultraviolet (FUV) observation of the Monogem ring made with the FIMS/SPEAR instrument. The global map constructed from the C IV λλ1548, 1550 emission lines reveals clear evidence of the interaction of the Monogem ring with the ambient medium. The image shows a half ring feature in the low latitude region, with its peak along the distorted boundary of the X-ray ring where the hot gas is in direct contact with the newly found Hα ring centered at (l, b) (191°.5, +5°.0). On the other hand, only a small portion of the X-ray ring is bright in C IV in the high latitude region where hot gas is seen to extend to a great distance from the ring. We have also detected other ionic emission lines in several regions of the Monogem ring such as C III λ 977, O VI λλ1032, 1038, Si II* λ 1533, He II λ 1640, and O III] λ 1666.

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