Calculate and plot the strength of the Balmer jump (i.e., the ratio of the opacities on either side of the 3647 Å limit) as a function of temperature for stars from 10,000 K to 30,000 K.
Calculate and plot the strength of the Balmer jump (i.e., the ratio of the opacities on either side of the 3647 Å limit) as a function of temperature for stars from 10,000 K to 30,000 K.
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Transcribed Image Text:Calculate and plot the strength of the Balmer jump (i.e., the ratio of
the opacities on either side of the 3647 Å limit) as a function of temperature for
stars from 10,000 K to 30,000 K.
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