Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1985
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985rpspr..12...51g&link_type=abstract
In its USSR Rept.: Space (JPRS-USP-85-005) p 51 (SEE N86-14111 04-88) Transl. into ENGLISH from Pisma v Astron. Zh. (Moscow),
Astronomy and Astrophysics
Astronomy
Density Wave Model, Gas Flow, Interstellar Gas, Milky Way Galaxy, Velocity Measurement, Flow Velocity, Mars 7 Spacecraft, Solar System, Spiral Galaxies, Venera 9 Satellite
Scientific paper
The measurements of the velocity of interstellar gas in the solar system obtained by the Mars 7 and Venera 9 probes (Bertaux et al., 1976 and 1978) are analyzed in the framework of the density-wave theory of spiral galaxies (Lin et al., 1969), assuming that the gas motion comprises a basic circular motion, a random component arising from a nearby disturbance such as a supernova outburst, and a systematic noncircular motion induced by the gravity field of a spiral density wave.
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