Aspects of Geneva photometry. Part 3 - Doing physics with colours

Details Aspects of Geneva photometry. Part 3 - Doing physics with colours Aspects of Geneva photometry. Part 3 - Doing physics with colours

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005orion..63a...4c&link_type=abstract

Orion (ISSN 0030-557X), 63. Jahrgang, No. 326, p. 4 - 12 (2005)

Physics

Geneva Photometry, Multicolor Photometry

Scientific paper

In this third part of the article, we consider the manner in which the multicolour photometric measurement can be calibrated in terms of primary data that, taken as a first example, is not sensitive to interstellar reddening. We consider the MK spectral classification as well as effective temperatures and bolometric corrections for the B-type stars. We also describe a good correlation between Geneva photometry and the Strömgren photometric Hβ index, leading to what we may call a "hyperindex" sensitive to emission in the Hβ line. Some unsuspected inconsistencies are revealed and briefly discussed.

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