An investigation of the structure of non-uniformities of interstellar absorption using photometry of globular clusters

Details An investigation of the structure of non-uniformities of interstellar absorption using photometry of globular clusters An investigation of the structure of non-uniformities of interstellar absorption using photometry of globular clusters

Jan 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004a%26at...23...35g&link_type=abstract

Astronomical and Astrophysical Transactions, vol. 23, Issue 1, p.35-41

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

Charge-coupled device photometric investigations of the central regions of the globular clusters NGC 4372 (r < 4') and NGC 6266 (0.5' < r < 2') were used to obtain detailed maps of the distribution of differential reddening. In both clusters the reddening is non-uniform on angular scales less than 1' and varies by magnitudes of 0.15 and 0.20 within the investigated fields of NGC 4372 and NGC 6266 respectively. For these clusters the average E(B - V) values of magnitudes 0.34 and 0.43 are smaller than those found previously.

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