Astrophysics II
Infrared spectroscopy is a technique used to identify and analyze the composition of matter by measuring how substances absorb infrared radiation. It is particularly useful in astrophysics for studying celestial objects, as it can reveal the presence of various molecules and dust in regions where visible light is blocked, such as in protostellar environments. This method allows astronomers to gather crucial information about the temperature, composition, and physical properties of young stellar objects and the surrounding material.
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