What is the orientation of the plane of M 33?

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astrometry, Astronomical Photometry, Density Wave Model, Galactic Structure, Spiral Galaxies, Astronomical Coordinates, Astronomical Photography, Axes Of Rotation, Galactic Rotation, Hydrogen Clouds, Stellar Evolution

Scientific paper

The discrepancy in M 33 inner region plane orientation values obtained from surface photometry data and data derived from the shape of the spiral is resolved by means of a two-step procedure. First, a V-band photograph of M 33 was scanned with a PDS microdensitometer, subtracting spiral arms and foreground stars by means of an automatic procedure. The results obtained are in agreement with those for the entire galaxy's surface photometry. Then, a detailed analysis of the spiral arms' delineation showed that the global form of the southern arm is due not only to stellar formation triggered by a shock wave, but also very active secondary star formation.

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