On linear fit to ZAMS and reddening determination.

Details On linear fit to ZAMS and reddening determination. On linear fit to ZAMS and reddening determination.

Oct 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996a%26a...314..108m&link_type=abstract

Astronomy and Astrophysics, v.314, p.108-111

Astronomy and Astrophysics

Astrophysics

24

Dust: Extinction, Open Clusters, Techniques: Photometric

Scientific paper

We re-discuss in detail the use of linear fit to the (B-V),(B-I) ZAMS of open clusters proposed by Natali et al. (1994) to measure the reddening. A proper link to the Cousins photometric system and evaluation of the adopted extinction law shows that the application of the proposed method must be carefully handled over observational data to avoid large errors. Other combinations of colors are explored in search for a higher sensitivity to reddening, which in any case remains quite poor.

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