The far-IR structure of the SNR G109.1 - 1.0

Details The far-IR structure of the SNR G109.1 - 1.0 The far-IR structure of the SNR G109.1 - 1.0

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.238..649c&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 238, May 15, 1989, p. 649-655. Research supported by Ca

Astronomy and Astrophysics

Astronomy

6

Far Infrared Radiation, Infrared Astronomy Satellite, Molecular Clouds, Pulsars, Supernova Remnants, X Ray Sources, Astronomical Maps, Binary Stars, Heao 2

Scientific paper

The raw IRAS scan data have been used to map the region of sky around and including the SNR G109.1 -1.0. This SNR is of particular interest because it contains the X-ray pulsar 1E2259 + 586 which is the only binary system apart from SS433 directly linked to an SNR. The results presented here confirm the strong interaction between the expanding SN shell and an adjacent molecular cloud complex. In addition, evidence is presented for the interaction of the apparent X-ray jet with material within the shell of the SNR.

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