On the extinction towards Baade's Window
Abstract
An analysis is made on the morphology of the sequences, formed by stars distributed along the line of sight in (V,V--I) colour-magnitude diagrams from Baade's Window (l=1.0,b=-3.9). The extinction is due to an absorbing layer with an effective thickness of about 100 pc. A linearly, with distance, increasing extinction up to a maximum value inside the absorbing layer is in first order a good approximation for the actual extinction present along the line of sight. We show that the morphology of the disc sequence gives a good indication of the nearby extinction along the line of sight. The morphology of the bulge/bar red horizontal branch is likely due to a combination of differential reddening and a significant metallicity spread among the horizontal branch stars. This is irrespective of the type of extinction law adopted. There is in Baade's Window globally no big difference between a Poissonian or a patchy type of extinction, except for substructures in the morphology of the sequences for the latter.
Cite
@article{arxiv.astro-ph/9607092,
title = {On the extinction towards Baade's Window},
author = {Y. K. Ng and G. Bertelli},
journal= {arXiv preprint arXiv:astro-ph/9607092},
year = {2007}
}
Comments
9 pages TeX without postscript figures (16), uses modified version of aa.cmm. Full paper, including all the postscript figures (approx. 15 Mb), is available on request. Accepted for publication in A&A