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Listen to native speakers pronounce “luminosity” in real conversational contexts with synchronized timestamps and subtitles.
We know its apparent brightness.We know the luminosity.We know its oomph.
We know the luminosity.
when we measured distance luminosity, distance versus redshift, was this curve.
in terms of luminosity and outline and texture and movement and depth.
The long exposure makes for the luminosity, and the clouds, and the water.
in their cores to sustain their luminosity, to shine, even for their short lives, they were expelled into the interstellar medium,
So that's just a luminosity distance.
So you need something of known luminosity.
That allows us to determine its true luminosity.
When you take into account this luminosity light curve shape relationship, and when you also take into account dust and other interstellar
by taking their spectra, luminosity, and by every possible means to understand what's going on there, what are the kinds of matter, in what
But you can extract domain-specific features like hue and luminosity.
They just wouldn't have the power and the luminosity and the impact.
But the confirmation of this light curve shape versus luminosity relationship with the Katzman telescope, so that was something we did.
So there's a disconnect here between the temperature that's observed and the luminosity of the object.
collecting detailed information on the soil conditions and ambient environment like temperature and luminosity, et cetera.
Spectrographs may be used to evaluate light, whereas photoelectric cells can be employed to measure luminosity.
And so they should explode in exactly the same way each time and reach the same peak luminosity.
measure their light curves, and figure out whether this is a normal luminosity one, an over luminous one, or a sub-luminous one.
And on the y-axis, we have absolute magnitude and luminosity.
We will define, what I will call it, luminosity distance in the stock.
The measurement of the brightness is easy, but how do you know the luminosity?
And the point is, you know what their true luminosity is.
The first reason is, by the observed brightness compared to the luminosity, you get the distance and hence the lookback time.
And there's a movement afoot, a successful movement, to change its name from the period luminosity relation
This is a titanic, colossal explosion that can make the star up to several billion times the brightness of our sun, or the luminosity,
So if you don't take that into account, and you're looking at some distant type 1a supernova, and you don't know the true luminosity,
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