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    The evolutionary track for a star of 1 solar mass remains nearly vertical in the H–R diagram for a while (see ). How is its luminosity changing during this time? Its temperature? Its radius?

    The course author didn't provide an answer for this question

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Source:  OpenStax, Astronomy. OpenStax CNX. Apr 12, 2017 Download for free at http://cnx.org/content/col11992/1.13
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