The kinematics of NGC 6164-5

Details The kinematics of NGC 6164-5 The kinematics of NGC 6164-5

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.123...59c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 123, no. 1, June 1986, p. 59-65.

Astronomy and Astrophysics

Astrophysics

Gas Dynamics, H Alpha Line, Nebulae, O Stars, Radial Velocity, Spectral Energy Distribution, Distance, Kinematics, Spatial Distribution, Spectrum Analysis, Velocity Distribution

Scientific paper

Accurate interferometric kinematic data suggest the interpretation of the brightest regions of NGC 6164-5 as a two-branched helical structure related to HC 148937 and having a systematic radial velocity nearly coincident with that of the tenuous surrounding medium; the gas in the helix could be the result of non-equatorial ejections from the central star. Morphologic, spectroscopic, and kinematic data would also indicate that the distance of 1.4 kpc proposed by Westerlund (1960) is substantially correct.

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