Possible association between the molecular and optical line splitting in M17, M8 and M16

Details Possible association between the molecular and optical line splitting in M17, M8 and M16 Possible association between the molecular and optical line splitting in M17, M8 and M16

Sep 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976a%26a....51..401g&link_type=abstract

Astronomy and Astrophysics, vol. 51, no. 3, Sept. 1976, p. 401-410.

Astronomy and Astrophysics

Astrophysics

31

H Lines, Hydrogen Clouds, Molecular Spectra, Radial Velocity, Hydrogen Ions, Ionized Gases, Solar Orbits

Scientific paper

Accurate heliocentric radial velocities have been derived for the regions of M8, M17, and M16 emitting the O III forbidden line. These have been compared in detail with those observed for the adjacent neutral masses of molecules, neutral hydrogen, and dust. Several interesting correlations emerge; in M17, the unusual motions of the neutral material appear to be closely related to those observed at optical wavelengths.

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