The neutral hydrogen west of lambda Orionis

Details The neutral hydrogen west of lambda Orionis The neutral hydrogen west of lambda Orionis

Oct 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980sval....6..303b&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 6, Sept.-Oct. 1980, p. 579-581.) Soviet Astronomy Letters, vol. 6, Sept.-Oct. 1980, p.

Astronomy and Astrophysics

Astronomy

Hydrogen Clouds, Interstellar Gas, Nebulae, Radio Emission, Astronomical Photography, Chemical Composition, Mass Distribution, Neutral Particles, Radial Velocity, Temperature Distribution

Scientific paper

The distribution of H I in the neighborhood of the two faint H-alpha filaments and loop near lambda Ori has been investigated. The pattern observed at velocities relative to the local standard of rest + 4.5, + 9.7, and, in part, + 15 km/sec suggests that the H I is associated with the optical filaments; but the proposed existence of a common expanding envelope of a relative thickness of about 0.6 is not confirmed.

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