Sensitive OH observations towards 16 supernova remnants

Details Sensitive OH observations towards 16 supernova remnants Sensitive OH observations towards 16 supernova remnants

May 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989mnras.238..737g&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 238, May 15, 1989, p. 737-751.

Astronomy and Astrophysics

Astronomy

39

Hydroxyl Emission, Line Spectra, Molecular Clouds, Radio Telescopes, Supernova Remnants, Radio Astronomy, Space Observations (From Earth)

Scientific paper

Sensitive observations made toward 16 supernova remnants in the 1.667-GHz OH line with the DRAO 26-m radio telescope are presented. These observations were made in a search for broad, asymmetric absorption features, such as that seen toward G189.1 + 3.0 (IC443), in order to identify remnants which are interacting with molecular clouds and producing shock-excited species. Absorption by shocked OH is indicated in the cases of G33.6 + 0.1 and G84.2 - 0.8. Useful constraints on distances to several remnants are also derived.

Affiliated with

Also associated with

No associations

Rating

Sensitive OH observations towards 16 supernova remnants does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Sensitive OH observations towards 16 supernova remnants, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Sensitive OH observations towards 16 supernova remnants will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1874867