pith. sign in

arxiv: astro-ph/9209001 · v2 · pith:3VY7NW24new · submitted 1992-09-04 · 🌌 astro-ph

The Radial Structure of the Galactic Disc

classification 🌌 astro-ph
keywords galacticcolourdatadiscabruptlyabsorptionanticenterarea
0
0 comments X
read the original abstract

Three colour photometry on CCD frames in the Special Area SpA23 provides a deep probe of the galactic disc in a low absorption window towards the anticenter. Magnitudes to better than 10% at V = 25 and B-V colour down to V = 23 have been obtained. These new data, used in combination with lower magnitude photographic data in a wider field, give a strong evidence that the galactic density scale length is rather short (2.5 kpc) and drops abruptly beyond 6 kpc.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.