Detection of interstellar CH and CH(+) towards SN 1987a

Details Detection of interstellar CH and CH(+) towards SN 1987a Detection of interstellar CH and CH(+) towards SN 1987a

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...184l...5m&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 184, no. 1-2, Oct. 1987, p. L5, L6.

Astronomy and Astrophysics

Astrophysics

12

Abundance, Free Radicals, Interstellar Matter, Magellanic Clouds, Methyl Compounds, Supernova 1987A, Light Sources, Line Spectra, Near Ultraviolet Radiation, Signal To Noise Ratios

Scientific paper

The authors report the detection of interstellar CH and CH+
towards supernova 1987A. For both of these molecules, one component is
detected at a heliocentric velocity of about 280 km/s, corresponding to
material inside the LMC. Some implications of the authors' results with
regards to the H2-to-dust ratio are briefly discussed.

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