<transcript><audio_68> ¿Cómo?</transcript><transcript><audio_69> tiene para clasificar o visualizar un grupo de estrellas. Un diagrama HR lo que hace es graficar, por así decirlo, o colocar las estrellas dentro, de acuerdo a</transcript><transcript><audio_70> su temperatura, que es lo que tenemos en el eje X, y su luminosidad. Esta línea que tenemos aquí es</transcript><caption><image_71>The image shows a man standing in front of a projector screen in a classroom. The screen displays a presentation slide with a map and text in Spanish. The text on the slide appears to be related to the presentation, as there is a title at the top of the screen and a subtitle at the bottom. The man is wearing a black shirt and is standing in a dimly lit room with a whiteboard and two shields on the wall behind him.</caption><transcript><audio_72> que tenemos aquí, esta línea sólida, corresponde a las estrellas jóvenes. Se les llama estrellas de secuencia principal. De hecho, por aquí tenemos estrellas</transcript><transcript><audio_73> ¿Por qué? Pues porque el Sol es una estrella de baja masa, es una estrella fría. Entonces, básicamente, estrellas tipo Sol corresponden a esta región del diagrama de</transcript><transcript><audio_74> Se le llama la región de inestabilidad. Y es cuando las estrellas van saliendo de ser jóvenes, es decir, jóvenes,</transcript> speak and the moment it which is like the way you have to classify or  visualize a group of stars an hr diagram what it does is graph so to speak or place the stars within according to their spectral type or their temperature which is what the line we have here this solid line the line we have here this solid line Corresponds to young stars, they are called main sequence stars. they are called main sequence stars. In fact, here we have solar-type stars because because it is only a low star, it is a cold star, so basically sun-type stars correspond to this region of the this line.  What we have here is called the region of instability and it is when the stars are coming out of being young, that is,
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