The galactic structure in the extreme ultraviolet (results and future programs)

Details The galactic structure in the extreme ultraviolet (results and future programs) The galactic structure in the extreme ultraviolet (results and future programs)

Jun 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978esasp.135..265s&link_type=abstract

In ESA European Sounding Rocket, Balloon and Related Res., with Emphasis on Expt. at High Latitudes p 265-266 (SEE N79-31637 2

Astronomy and Astrophysics

Astronomy

Galactic Structure, Milky Way Galaxy, Ultraviolet Astronomy, Ultraviolet Photography, Astronomical Coordinates, Spiral Galaxies, Statistical Analysis, Wide Angle Lenses

Scientific paper

Wide-angle photographs of our galaxy reveal the fine structure of the
arms 0, -I and -II. The axis of each spiral arm shows a characteristic
pattern b = b(1), which may be used for statistical distance
determinations. The mean deviation of spiral tracers from the arm axis
decreases with decreasing wavelength and is only 12 per cent at 2900 A.

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