<transcript><audio_94> Cuando hablamos de las observaciones espectrales, estamos hablando de un espectrógrafo de baja resolución al principio, entonces lo que queremos hacer con estos espectros es poder ajustarlos a algún modelo de atmósfera estelar.</transcript><transcript><audio_95> Mae llawer o fodelau o amgylcheddau estelares. Mae rhai wedi'u datblygu yng Nghymru gan y grŵp Phoenix, mae eraill wedi'u datblygu yng Nghymru, mae'n atlas gan Crux ym 1993.</transcript><transcript><audio_96> espectros de atmósferas estelares no crean que los desarrollaron por ejemplo en el 93 y ahí se quedaron no, todos estos modelos permiten cambios, entonces se les puede ir modificando, ya sea</transcript> when we talk about spectral observations we are talking about a low resolution spectrograph at the beginning so what we want to do with  These spectra are to be able to adjust them to some model of the stellar atmosphere. adjust them to some model of the stellar atmosphere. Right now there are many models of the stellar atmosphere. There are some developed in Germany by the Phoenix group. There are others developed in the United States. It is an upcoming one in the atlas. of stellar atmospheres, do not believe that they developed them, for example in 93, and they stayed there. Not all of these models allow changes, so they can be modified
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