The Distances to Nearby Galaxies from Near Infrared Photometry

Details The Distances to Nearby Galaxies from Near Infrared Photometry The Distances to Nearby Galaxies from Near Infrared Photometry

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985cto..conf..228m&link_type=abstract

Cepheids: Theory and Observations, Proceedings of IAU Colloquium No. 82, held 29 May - 1 June, 1984 in Toronto, Canada. Edited

Physics

5

Scientific paper

Near-infrared photometry of Cepheid variables in the Local Group
galaxies, NGC 6822, IC 1613, and M33, and in the M81 Group galaxy, NGC
2403 has been used to determine new, independent distances to these
objects, which are almost unaffected by dust extinction and by
differences in metallicities among the galaxies.

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