Mass-luminosity relation
When the luminosity of main sequence stars is plotted against their masses, we observe a mass‐luminosity relationship, approximately of the form L ∝ M 3.5 (see Figure ). In other words, doubling the mass of a main sequence star produces an increase in lum,2022年6月19日 — Furthermore, the luminosity depends on the mass raised to a power that is between three and four (Luminosity ~ Massp, where p is between 3 & 4).
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 Mass-luminosity relation 相關參考資料
How Does A Star’s Mass Determine The Mass Luminosity ...
When the luminosity of main sequence stars is plotted against their masses, we observe a mass‐luminosity relationship, approximately of the form L ∝ M 3.5 (see Figure ). In other words, doubling the m... https://www.youtube.com Mass Luminosity Relationship - Astronomy - CliffsNotes
When the luminosity of main sequence stars is plotted against their masses, we observe a mass‐luminosity relationship, approximately of the form L ∝ M 3.5 (see Figure ). In other words, doubling the m... https://www.cliffsnotes.com Mass-Luminosity Relation Explained
2022年6月19日 — Furthermore, the luminosity depends on the mass raised to a power that is between three and four (Luminosity ~ Massp, where p is between 3 & 4). https://www.astronomynotes.com Mass-luminosity relation of intermediate-mass stars
由 OY Malkov 著作 · 2007 · 被引用 146 次 — Abstract. The mass-luminosity relation (MLR) for intermediate-mass stars is based on data on detached double-lined eclipsing binaries. http://ui.adsabs.harvard.edu Mass–luminosity relation
In astrophysics, the mass–luminosity relation is an equation giving the relationship between a star's mass and its luminosity, first noted by Jakob Karl ... https://en.wikipedia.org Revisiting the mass-luminosity relation with an effective ...
由 J Wang 著作 · 2018 · 被引用 18 次 — The mass-luminosity relation (MLR) is commonly used to estimate the stellar mass. The classical MLR can hardly fit data of all the stellar mass range, thus ... https://www.aanda.org Stellar Masses
This mass-luminosity relationship is considered one of the most fundamental descriptions of stellar properties; the ability to reproduce this by stellar models ... http://www2.lowell.edu The Mass-Luminosity Relationship | Astronomy 801
The more massive a star, the faster it lives its lifetime, and, given the exponent of this relationship, it isn't a linear relationship. https://www.e-education.psu.ed |