The model was valid at high interstellar absorption.
2.
Interstellar absorption in other galaxies can similarly be described by fairly simple'laws '.
3.
True distance moduli require a further theoretical step, that is the estimation of the interstellar absorption coefficient.
4.
NGC 3603 is visible in the telescope as a small rather insignificant nebulosity with a yellowish tinge due to the effects of interstellar absorption.
5.
Thus a distinction is made between distance moduli uncorrected for interstellar absorption ( whose values would overestimate the distance if used naively ) and absorption-corrected moduli.
6.
While this is partly due to interstellar absorption, any tight clustering of stars at such a great distance in the galactic plane would be scarcely distinguishable from the general background.
7.
Due to interstellar absorption of light, the distance to "'M52 "'is uncertain, with estimates ranging between 3, 000 and 7, 000 light years.
8.
The distance modulus \ mu = m-M is the difference between the apparent magnitude m ( ideally, corrected from the effects of interstellar absorption ) and the absolute magnitude M of an astronomical object.
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