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Luminosity-color variation: Improve explanation of the enlargement of aging stars
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Add: bibcode, authors 1-1. Removed parameters. Some additions/deletions were parameter name changes. | Use this bot. Report bugs. | Suggested by Abductive | Category:Concepts in astronomy | #UCB_Category 68/71
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* [[K-type main-sequence star]]
* [[M-type main-sequence star]]
M-type (and, to a lesser extent, K-type)<ref>{{Cite journal |lastlast1=Pettersen |firstfirst1=B. R. |last2=Hawley |first2=S. L. |date=1989-06-01 |title=A spectroscopic survey of red dwarf flare stars. |url=https://ui.adsabs.harvard.edu/abs/1989A&A...217..187P |journal=Astronomy and Astrophysics |volume=217 |pages=187–200 |bibcode=1989A&A...217..187P |issn=0004-6361}}</ref> main-sequence stars are usually referred to as [[Red dwarf|red dwarfs]].
 
==Properties==