Lecture

Spectral Classification: Introduction to Astrophysics

In course
DEMO: commodo eiusmod nisi voluptate
Qui est ad veniam excepteur elit esse quis Lorem officia eu irure exercitation. Mollit anim labore laboris ex dolor commodo pariatur elit. Eiusmod dolore eiusmod in do sit dolore nisi id minim. Officia laborum incididunt excepteur in aute tempor.
Login to see this section
Description

This lecture covers the spectral classification of stars based on their temperature and flux, introducing the types B, A, F, G, K, and M. It explains how the temperature affects the spectral types and the flux, providing insights into the classification of stars in the universe.

Instructor
aute est
Lorem enim cillum incididunt adipisicing ut ex consectetur do deserunt. Sit officia elit nisi ut culpa duis excepteur aliquip. Aliquip qui culpa enim cupidatat consectetur dolore Lorem nisi voluptate dolor occaecat culpa. Commodo velit sint excepteur adipisicing enim fugiat sunt aliqua incididunt sunt sunt. Aliquip nisi Lorem nulla esse. Eiusmod eiusmod est Lorem cillum commodo reprehenderit culpa quis amet reprehenderit id proident minim pariatur.
Login to see this section
About this result
This page is automatically generated and may contain information that is not correct, complete, up-to-date, or relevant to your search query. The same applies to every other page on this website. Please make sure to verify the information with EPFL's official sources.