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Cosmic chemical evolution and diffuse background radiation

To explain this, we must consider that, from the known velocity of light, it may be proved, that when we look at Sirius, the rays which enter the eye cannot have been less than 6 years and 4 months coming from that star to the observer. Hence it follows, that when we see an object of the calculated distance at which one of these very remote nebulae may still be perceived, the rays of light which convey its image to the eye, must have been more than nineteen hundred and ten thousand, that is, almost two millions of years on their way and that, consequently, so many years ago, this object must already have had an existence in the sidereal heavens, in order to send out those rays by which we now perceive it. [Pg.374]

William Herschel, Catalogue of500 new Nebulae, nebulous stars, planetary Nebulae, and Clusters of Stars with Remarks on the [Pg.374]

Observations of distant objects, notably high-redshift star-forming ( Lyman-break ) galaxies and absorption line systems on the line of sight to quasars, give some information on chemical evolution at epochs not too far from when the first stars and most galaxies were presumably formed. Other information comes from two related effects  [Pg.374]


Cosmic chemical evolution and diffuse background radiation... [Pg.374]




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Background radiation

Chemical background

Cosmic

Cosmic Background

Cosmic chemical evolution

Cosmics

Diffuse background

Diffuse background radiation

Diffusivity chemical

Evolution radiation

Evolution, chemical

Radiation diffuse

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