A search for SH(+) toward Zeta Ophiuchi

Details A search for SH(+) toward Zeta Ophiuchi A search for SH(+) toward Zeta Ophiuchi

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988mnras.231..953m&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 231, April 15, 1988, p. 953-955.

Astronomy and Astrophysics

Astronomy

8

Magnetohydrodynamic Waves, Methyl Compounds, Molecular Clouds, Molecular Ions, Ophiuchi Clouds, Shock Waves, Chemical Reactions, Electron Transitions, Interstellar Magnetic Fields, Line Of Sight, Spectral Resolution, Sulfur Compounds

Scientific paper

The authors have searched toward ζ Ophiuchi for interstellar absorption from the R11(0) line in the A3Π - X3Σ-(0-0) band of SH+ at a wavelength of 3363.49 Å in a new observational test of recent magnetohydrodynamical shock models. They have derived a low upper limit to the equivalent width of this line, Wλ(3σ) = 0.64 mÅ, and discuss the implications of this result.

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