Towards using optical/NIR photometry to measure the temperature of O stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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2 pages, to appear in Massive Stars: Fundamental Parameters and Circumstellar Interactions

Scientific paper

It has been traditionally stated that it is not possible to use optical/NIR
photometry to measure the temperatures of O stars. In this contribution we
describe the steps required to overcome the hurdles that have prevented this
from happening in the past and we present our preliminary results for the
low-extinction case.

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